/openshift/adei-setups/asec : revision 1.1.1

To get this branch, use:

bzr branch
http://darksoft.org/webbzr/openshift/adei-setups/asec

« back to all changes in this revision

Viewing changes to wiki.xml

Committer: Suren A. Chilingaryan
Date: 2020-02-05 08:53:51 UTC
mto: This revision was merged to the branch mainline in revision 2.
Revision ID: csa@suren.me-20200205085351-j85b2s444mycsr04

Update for KaaS (exlcuding graph-related stuff for now)

files added:
classes

classes/drawexport.php

classes/handlers

classes/handlers/histogram.php

classes/handlers/image.php

classes/readers

classes/readers/crdreader.php

classes/views

classes/views/calcview.php

classes/views/correlationsview.php

classes/views/histogramview.php

classes/views/integralview.php

classes/views/scatterview.php

crd.gif

modules

modules/export.php

pictures/300px_STAND_3cm.jpg

pictures/ADEI_Publication.pdf

pictures/Efficiencies.pdf

pictures/PCIBoardAntenna92-StormTracker.png

pictures/STAND_3cm.jpg

pictures/WeatherStation1.JPG

pictures/WeatherStation1_small.JPG

pictures/WeatherStationSpecifications.pdf

pictures/WeatherStationVariables.pdf

pictures/background_btn.png

pictures/ld_button.png

pictures/sky_button.png

xslt

xslt/views

xslt/views/correlations.xsl

xslt/views/integral.xsl

xslt/views/legend.xsl

files removed:
config.php.main

config.php.mirror

files modified:
asec.css

config.php

wiki.xml

Show diffs side-by-side

added added

removed removed

wiki.xml

<!--<<>><pages>

<page id="0" title="">[[Main Page]][br]

</page>

<page id="1" title="Main Page">!ASEC Advanced Data Extraction Infrastracture of the ASEC

Dear user, welcome to the ASEC Advanced Data Extraction Infrastructure! The ASEC ADEI is loaded and ready to work. Please, click on [u][b]"Data Source"[/b][/u] popup

on the left sidebar and select the data [i][b]Source[/b][/i] and [i][b]Time[/b][/i] interval. Alternatively, you could use a pulldown [u][b]"Menu"[/b][/u] on the top

of sidebar.

Navigation through the data is feasible with mouse. Please, press and hold left mouse button to select region. Then click on the arrow button to zoom inside. The

mouse wheel could be used to shift current window left.

To [b]download[/b] selected data open [u][b]"Controls"[/b][/u] popup and choose [i][b]"Export"[/b][/i] tab. You will be able to get the data in the multiple supported

formats. Please, Be patient, the preparation of data may take a while.

More detail description, how to use ADEI, you can find in [b][[Users Guide]][/b]

To find more information about ADEI system and report bugs, please, visit [url="http://dside.dyndns.org/adei"]project home page[/url].

Below, you will find, [b]Description of the monitors[/b] and their data, presented in this site.

<page id="1" title="Main Page">![U]A[/u]dvanced [u]D[/u]ata [u]E[/u]xtraction [u]I[/u]nfrastructure of [u]A[/u]ragats [u]S[/u]pace [u]E[/u]nvironmental [u]C[/u]enter (ADEI of ASEC)

Dear user, welcome to the ASEC Advanced Data Extraction Infrastructure! The ASEC ADEI is loaded and ready to work.

Please select the data [i][b]Source[/b][/i] and [i][b]Time[/b][/i] interval from the [i][b]Data Source[/b][/i] popup on the left sidebar, or use the pulldown menu in the top-left corner.

Navigation through the data done with the mouse:

*Drag with left mouse button to select a region.

*Click on the arrow button to zoom inside a region.

*Use the mouse wheel shift current window left and right.

To [b]download[/b] selected data open choose the [i][b]Export[/b][/i] tab from [i][b]Controls[/b][/i] popup. You can export data to the multiple supported formats. Please be patient, as exporting data may take a while.

More detailed information about how to use ADEI can be found in the [b][[Users Guide|ADEI Users' Guide]][/b].

To find more information about ADEI system and report bugs, please, visit [url="http://adei.info"]project home page[/url].

Please read [url="setups/asec/pictures/ADEI_Publication.pdf"]this[/url] publication to get more information how is working ADEI.

[url="setups/asec/pictures/Efficiencies.pdf"]The Efficiencies of the ASEC particle detectors used in

Thunderstorm Ground Enhancement (TGE) research (Bagrat Mailyan)[/url]

Below you will find [b]descriptions of the monitors[/b] and their data.

{| border="1px"

[u][b][[Aragats Research Station]] (40.47N, 44.18E, 3200m a.s.l.)[/b][/u] || [u][b][[SEVAN Monitors]][/b][/u]

[[AMMM]] - Aragats Multichannel Muon Monitor [br]

[[ArNM]] - Aragats Neutron Monitor [br]

[[ASNT]] - Aragats Solar Neutron Telescope [br]

[[Boltek EFM100 Aragats]] - Electric Field Monitor at Aragats [br]

[[Boltek LD Aragats]] - Lightning Detector at Aragats [br]

[[Cube]] - Monitor of the neutral cosmic ray fluxes [br]

[[Lemi-417]] - Magnetotelluric Station (MTS) [br]

[u][b][[Aragats Research Station]] ([url="https://maps.google.com/maps?q=40.4715N,44.1815E"]40.47N, 44.18E[/url], 3200m a.s.l.)[/b][/u]

[[AMMM]] - [b]A[/b]ragats [b]M[/b]ultichannel [b]M[/b]uon [b]M[/b]onitor [br]

[[ArNM]] - [b]A[/b]ragats [b]N[/b]eutron [b]M[/b]onitor [br]

[[ASNT]] - [b]A[/b]ragats [b]S[/b]olar [b]N[/b]eutron [b]T[/b]elescope [br]

[[Cube]] - Neutral Cosmic Ray Monitor [br]

[[MAKET]] - MAKET-ANI Extensive Air Shower Detector [br]

[[NaI]] - NaI(Tl) Monitor [br]

[[SEVAN Aragats]] - SEVAN network Monitor at Aragats [br]

[[Stand]] - Monitor of low energy particles [br]

[[Stand_3cm]] - Monitor with possibility to estimate energy of particles [br]

[[Weather Station]] - Vantage Pro 2 Weather Station [br]

[u][b][[NorAmberd Research Station]] (40.37N, 44.26E, 2000m a.s.l.)[/b][/u]

[[Boltek EFM100 NorAmberd]] - Electric Field Monitor at NorAmbed [br]

[[Boltek LD NorAmberd]] - Lightning Detector at NorAmbed [br]

[[Magnetometer]] - Magnetotelluric Station (MTS) Lemi-018 [br]

[[NAMMM]] - NorAmberd Multidirectional Muon Monitor [br]

[[NANM]] - NorAmberd Neutron Monitor [br]

[[SEVAN NorAmberd]] - SEVAN network Monitor at NorAmberd [br]

[u][b][[Yerevan CRD headquarters]] (40.20N, 44.49E, 1090m a.s.l.)[/b][/u]

[[Boltek EFM100 Yerevan]] - Electric Field Monitor at NorAmbed [br]

[[Boltek LD Yerevan]] - Lightning Detector at NorAmbed [br]

[[SEVAN]] - SEVAN Monitor at Aragats [br]

[[Stand 1cm|Stand 1cm]] - Plastic Scintillator Monitor for Low Energy Particles [br]

[[Stand_3cm|Stand 3cm]] - Plastic Scintillator Monitor with Spectral Analysis [br]

[[Electric Field]] - Electric Field Monitor at Aragats [br]

[[Lightning Detector]] - Lightning Detector at Aragats [br]

[[LEMI-417]] - Magnetotelluric Station (MTS) [br]

[[Weather Station]] - Davis Wireless Vantage Pro2 Plus [br]

[u][b][[Nor-Amberd Research Station]] ([url="https://maps.google.com/maps?q=40.375N,44.2642E"]40.37N, 44.26E[/url], 2000m a.s.l.)[/b][/u]

[[NAMMM]] - [b]N[/b]or-[b]A[/b]mberd [b]M[/b]ultidirectional [b]M[/b]uon [b]M[/b]onitor [br]

[[NANM]] - [b]N[/b]or-[b]A[/b]mberd [b]N[/b]eutron [b]M[/b]onitor [br]

[[SEVAN]] - SEVAN Monitor at Nor-Amberd [br]

[[Electric Field]] - Electric Field Monitor at Nor-Amberd [br]

[[Lightning Detector]] - Lightning Detector at Nor-Amberd [br]

[[LEMI-018]] - Magnetotelluric Station (MTS) [br]

[[Weather Station]] - Davis Wireless Vantage Pro2 Plus [br]

|| [u][b][[Yerevan CRD headquarters]] ([url="https://maps.google.com/maps?q=40.2046N,44.4857E"]40.205N, 44.486E[/url], 1090m a.s.l.)[/b][/u]

[[SEVAN]] - SEVAN Monitor at Yerevan [br]

[[Electric Field]] - Electric Field Monitor at Nor-Amberd [br]

[[Lightning Detector]] - Lightning Detector at Nor-Amberd [br]

[[Cube_3cm]] - Magnetotelluric Station (MTS) [br]

[[SEVAN Yerevan]] - SEVAN network Monitor at Yerevan [br]

[[SEVAN Burakan]] - SEVAN network Monitor at Burakan [br]

[[SEVAN Aragats]] - SEVAN network Monitor at Aragats [br]

[[SEVAN NorAmberd]] - SEVAN network Monitor at NorAmberd [br]

[[SEVAN Yerevan]] - SEVAN network Monitor at Yerevan [br]

[[SEVAN Burakan]] - SEVAN network Monitor at Burakan [br]

[[SEVAN Moussala]] - SEVAN network Monitor at Moussala [br]

[[SEVAN Zagreb]] - SEVAN network Monitor at Zagreb [br]

[[SEVAN JNU]] - SEVAN network Monitor at New Delhi University [br] [br]

[[Weather Station]] - Davis Wireless Vantage Pro2 Plus [br]

[u][b][[Sevan Lake]] ([url="https://maps.google.com/maps?q=40.61915N,45.02838E"]40.619N, 45.028E[/url], 1910m a.s.l.)[/b][/u]

[[Stand 1cm|Stand 1cm]] - Plastic Scintillator Monitor for Low Energy Particles [br]

[[Electric Field]] - Electric Field Monitor at Nor-Amberd [br]

[[Lightning Detector]] - Lightning Detector at Nor-Amberd [br]

[u][b][[SEVAN|SEVAN Monitors]][/b][/u]

SEVAN Aragats - SEVAN Monitor at Aragats [br]

SEVAN Nor-Amberd - SEVAN Monitor at Nor-Amberd [br]

SEVAN Yerevan - SEVAN Monitor at Yerevan [br]

SEVAN Byurakan - SEVAN Monitor at Byurakan [br]

SEVAN Moussala - SEVAN Monitor at Moussala [br]

SEVAN Zagreb - SEVAN Monitor at Zagreb [br]

SEVAN JNU - SEVAN Monitor at Jawaharlal Nehru University, New Delhi, India [br] [br]

[u][b][[TGE|List of TGE Events]][/b][/u]

[u][b]Data Overview[/b][/u] [br]

[[Channel List]] - List of all available channels alphabetically [br]

[[Group List]] - List of all available channels by groups [br]

[[Graph Preview]] - Preview charts of available groups [br]

[[Pressure Preview]] - Preview charts of Pressure Sensors [br]

</page>

<page id="2" title="Channel List">!Channel List | [[Main Page]]

[channels_by_name]

return back to [[Main Page]]

</page>

<page id="3" title="Group List">!Channel List | [[Main Page]]

103

116

104

117

return back to [[Main Page]]

105

118

</page>

106

107

119

<page id="6" title="Pressure Preview">!!Pressure Preview | [[Main Page]]

108

120

109

121

Pressure for last [u][i][b]1 Hour[/b][/i][/u] [br]

110

[preview(db_server=asec&amp;db_name=crd&amp;db_group=pressure_view&amp;db_mask=0&amp;width=600&amp;height=200&amp;window=3600), link]

122

[preview(db_server=ar&amp;db_name=raw&amp;db_group=Weather_Station_AR&amp;db_mask=14&amp;width=600&amp;height=200&amp;window=3600), link]

111

123

112

124

Pressure for last [u][i][b]6 Hour[/b][/i][/u] [br]

113

[preview(db_server=asec&amp;db_name=crd&amp;db_group=pressure_view&amp;db_mask=0&amp;width=600&amp;height=200&amp;window=21600), link]

125

[preview(db_server=ar&amp;db_name=raw&amp;db_group=Weather_Station_AR&amp;db_mask=14&amp;width=600&amp;height=200&amp;window=21600), link]

114

126

115

127

Pressure for last [u][i][b]Day[/b][/i][/u] [br]

116

[preview(db_server=asec&amp;db_name=crd&amp;db_group=pressure_view&amp;db_mask=0&amp;width=600&amp;height=200&amp;window=86400), link]

128

[preview(db_server=ar&amp;db_name=raw&amp;db_group=Weather_Station_AR&amp;db_mask=14&amp;width=600&amp;height=200&amp;window=86400), link]

117

129

118

130

Pressure for last [u][i][b]Week[/b][/i][/u] [br]

119

[preview(db_server=asec&amp;db_name=crd&amp;db_group=pressure_view&amp;db_mask=0&amp;width=600&amp;height=200&amp;window=604800), link]

131

[preview(db_server=ar&amp;db_name=raw&amp;db_group=Weather_Station_AR&amp;db_mask=14&amp;width=600&amp;height=200&amp;window=604800), link]

120

132

121

133

Pressure for last [u][i][b]Month[/b][/i][/u] [br]

122

[preview(db_server=asec&amp;db_name=crd&amp;db_group=pressure_view&amp;db_mask=0&amp;width=600&amp;height=200&amp;window=2592000), link]

134

[preview(db_server=ar&amp;db_name=raw&amp;db_group=Weather_Station_AR&amp;db_mask=14&amp;width=600&amp;height=200&amp;window=2592000), link]

123

135

124

136

Pressure for last [u][i][b]Year[/b][/i][/u] [br]

125

[preview(db_server=asec&amp;db_name=crd&amp;db_group=pressure_view&amp;db_mask=0&amp;width=600&amp;height=200&amp;window=31536000), link]

137

[preview(db_server=ar&amp;db_name=raw&amp;db_group=Weather_Station_AR&amp;db_mask=14&amp;width=600&amp;height=200&amp;window=31536000), link]

126

138

127

139

128

140

[[Main Page]]

129

141

</page>

130

131

132

133

134

135

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

136

[f] [[Main Page]][/f]

142

143

144

145

146

[f] [b][[Main Page|Return to Main Page]][/b][/f]

137

147

138

148

139

149

!About Aragats Research Station

144

154

[i][b]Figure 1:[/b] Aragats Station, altitude 3200m above sea level.[/i]

145

155

146

156

147

Cosmic Ray research at high altitude stations on Mt. Aragats, Armenia, was founded by famous Armenian physicists, Alikhanyan brothers, in 1943. Research facilities are located on

148

two high-altitude stations on Mt.Aragats, Nor-Amberd (40.37N, 44.26E, 2000m above sea level) Station and Aragats Station (40.47N, 44.18E, 3200m above sea level), and at CRD

149

headquarters at A.I. Alikhanyan National Science Laboratory, Yerevan.

150

151

152

153

154

155

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

156

[f] [[Main Page]][/f]

157

The cosmic ray research stations on Mt. Aragats, Armenia, were founded in 1943 by

158

[url="https://en.wikipedia.org/wiki/Artyom_Alikhanian"]Artyom Alikhanyan[/url] and

159

[url="https://en.wikipedia.org/wiki/Abraham_Alikhanov"]Abraham Alikhanov[/url],

160

famous Armenian physicist brothers. The Aragats Research Station ([url="https://maps.google.com/maps?q=40.4715N,44.1815E"]40.47N, 44.18E[/url], 3200m a.s.l.) is one of two high-altitude research facilities located on Mt. Aragats; it is complemented by [[Nor-Amberd Station]] ([url="https://maps.google.com/maps?q=40.375N,44.2642E"]40.37N, 44.26E[/url], 2000m a.s.l.) [br]

161

162

!Geography and Climate

163

164

Aragats Research Station is located on Mt. Aragats, a dormant stratovolcano in central Armenia, approximately 50 km (30 mi) northwest of Yerevan, Armenia. The youngest lava flows date between the late-Pleistocene and 3000 BCE (Kharakanian et al., 2003). As such, the station is located on solid volcanic rock foundations. At 3200m a.s.l., the Aragats Research Station lies above the tree line, on the shore of the man-made Lake Kari. [br]

165

166

At the Aragats Research Station, the average winter temperature is around -15 °C (5 °F), with temperatures occasionally reaching as low as -40 °C (-40 °F); during the summer, the average temperature is 12 °C (54 °F), with highs up to 20 °C (85 °F). Throughout the year, the humidity is between 72% and 80%. Average winds range from 20 km/hr (10 mph) in the summer to 40 km/h (20 mph) in winter, with occasional gusts up to 150 km/h (90 mph). For around 250 days each year, 1.65m of snow covers the ground.[br]

167

168

!Infrastructure

169

170

The Aragats Research Station has everything necessary of year-round operation. Mains power is available to the station, with diesel generators waiting on stand-by in case of loss of power. Detectors and their electronics are supported by servers and network connections to Yerevan. Staff spend one month shifts at the station; they have conference rooms, heated dormitories and a restaurant at their disposal.

171

172

[br]

173

{| border="1px"

174

[i][b]Figure 2a:[/b] Current horizion at Aragats Station.[/i]

175

176

[img]http://crd.yerphi.am/files/ASEC_Alert/AllSkyCam_Aragats/last_full_pano.jpg[/img]

177

178

[i][b]Figure 2b:[/b] Current sky above Aragats Station.[/i]

179

180

[img]http://crd.yerphi.am/files/ASEC_Alert/AllSkyCam_Aragats/last_full_raw.jpg[/img]

181

182

183

184

185

186

187

188

[f] [b][[Main Page|Return to Main Page]][/b][/f]

157

189

</page>

158

159

160

161

162

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

163

[f] [[Main Page]][/f]

190

191

192

193

194

[f] [b][[Main Page|Return to Main Page]][/b][/f]

164

195

165

196

166

197

!Aragats Multichannel Muon Monitor (AMMM)

167

198

168

The [b]A[/b]ragats [b]M[/b]ultichannel [b]M[/b]uon [b]M[/b]onitor ([b]AMMM[/b]) in operation at Aragats Station (40.47N, 44.18E, 3200m above sea level). AMMM consists

169

from 2 layers of the scintillation detectors. 29 scintillation detectors (each detector have 1m surface and 5cm thickness), located on top of the top

170

of ANI concrete calorimeter and 90 the same type detectors 14 m below (under 4m concrete and 7m soil), as shown in Figure 1 and Figure 2. Zenith angle between axes

171

of AMMM and direction to South pole is ~-17. Count rate in the upper detectors is ~28000 counts per minute and variance ~170. Count rate of each of

172

1m scintillators in the underground hall (high energy muons with energy threshold 5 GeV) is ~3000 counts per minute and variance ~55. The relative

173

accuracy of 1-minute count rates of underground high energy muon detector is ~0.2%, of the low energy muons and electrons on surface ~ 0.12%.

174

175

176

{| border="1px"

199

The [b]A[/b]ragats [b]M[/b]ultichannel [b]M[/b]uon [b]M[/b]onitor ([b]AMMM[/b]) is in operation at [[Aragats Research Station]]. The AMMM consists of 2 layers of scintillation detectors: 29 identical scintillation detectors are located above the ANI concrete calorimeter laid out on a 40m x 40m plane, and 90 scintillation detectors are located 24m below (under 4m of concrete, 6m of air, and 7m of soil) laid out in an 11m x 11m grid, as shown in Figure 1 and Figure 2. Each scintillation detector is a plastic slab with dimensions 1m x 1m x 5cm, with a photomultiplier tube to collect the scintillation light. The entire installation is rotated from the north-south axis by approximately 17°. [br]

200

201

The mean count rate in the upper detectors is 28000±170. The mean count rate of each of 1m scintillators in the underground hall (corresponding to high energy muons with energy &#62;5 GeV) is 3000±55. The relative efficiency of the underground detectors is ~0.2% for high-energy muons; the relative efficiency of the upper detectors is ~0.12% for low-energy muons and electrons.

202

203

204

205

{| border="1px" style="padding:2px"

177

206

[url="setups/asec/pictures/612px-AMMM.jpg"][img]setups/asec/pictures/350px-AMMM.jpg[/img][/url] ||

178

207

[url="setups/asec/pictures/AMMM_fig2.png"][img]setups/asec/pictures/350px-AMMM_fig2.png[/img][/url]

179

208

180

[i][b]Figure 1:[/b]Aragats Multidirectional Muon Monitor (AMMM).[/i] ||

181

[i][b]Figure 2:[/b]Projection of the AMMM on the X-Y plane.[/i]

209

[i][b]Figure 1:[/b] Aragats Multidirectional Muon Monitor (AMMM).[/i] ||

210

[i][b]Figure 2:[/b] Projection of the AMMM on the X-Y plane.[/i]

182

211

183

212

184

213

185

186

187

188

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

189

[f] [[Main Page]][/f]

214

215

216

217

218

[f] [b][[Main Page|Return to Main Page]][/b][/f]

190

219

</page>

191

192

193

194

195

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

196

[f] [[Main Page]][/f]

220

221

222

223

224

[f] [b][[Main Page|Return to Main Page]][/b][/f]

197

225

198

226

199

227

!Aragats Neutron Monitor (ArNM)

200

228

201

[b]Ar[/b]agats [b]N[/b]eutron [b]M[/b]onitor ([b]ArNM[/b]) in operation at Aragats Station (40.47N, 44.18E, 3200m above sea level) since 2000 year. Neutron Monitore consist

202

from NM-64 type 18 counter tubes (Moderator: Polyethylene, Reflector: Polyethylene, 3 sections by 6 counters). The monitor is equipped with electronics providing time

203

integration of counts by three dead times. The first dead time equals to 400ns for collecting almost all secondary neutrons generated in the lead of NM. The second dead

204

time is equal to the 0.25ms and the third one equal 1.25ms (as most of NM from world-wide network).

229

The [b]Ar[/b]agats [b]N[/b]eutron [b]M[/b]onitor ([b]ArNM[/b]) has been in operation at [[Aragats Research Station]] since 2000. The ArNM based on the 18-tube [url="http://www.nmdb.eu/?q=node/142"]NM64 neutron monitor[/url] design. The 18 counter tubes are filled with [sup]10[/sup]B-enriched boron-trifluoride (BF[sub]3[/sub]) gas, and detect neutrons by the ionization of the gas resulting from the exothermic reaction of the neutron and [sup]10[/sup]B to produce [sup]7[/sup]Li and [sup]4[/sup]He. In order to increase the efficiency of the ArNM, incoming particles are moderated by 6cm of polyethylene. The tubes themselves wrapped in lead to enhance the count rate by the [sup]210[/sup]Pb(n,2n) reaction, followed by another layer of polyethylene moderator 2cm thick. [br]

230

231

The monitor electronics provide time integration of counts for three dead times. The first dead time is 400ns, which collects almost all secondary neutrons generated in the lead producer of the ArNM. The second and third dead times are 0.25ms and 1.25ms (as with most of the NM64 world-wide network).

205

232

206

233

{| border="1px"

207

[url="setups/asec/pictures/800px-ArNM.jpg"][img]setups/asec/pictures/300px-ArNM.jpg[/img][/url] ||

208

[preview(db_server=nmdb&amp;db_name=crd&amp;db_group=nmdb_filtered&amp;db_mask=4&amp;width=560&amp;height=300&amp;window=86400), link]

234

[url="setups/asec/pictures/800px-ArNM.jpg"][img]setups/asec/pictures/800px-ArNM.jpg[/img][/url]

209

235

210

[i][b]Figure 1:[/b] Aragats Neutron Monitor (ArNM).[/i] ||

211

ArNM, Pressure corrected, Filtered data for last [u][i][b]Day[/b][/i][/u] [br]

236

[i][b]Figure 1:[/b] Aragats Neutron Monitor (ArNM).[/i]

212

237

213

238

214

239

215

216

217

218

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

219

[f] [[Main Page]][/f]

240

241

242

243

244

[f] [b][[Main Page|Return to Main Page]][/b][/f]

220

245

</page>

221

222

223

224

225

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

226

[f] [[Main Page]][/f]

246

247

248

249

250

[f] [b][[Main Page|Return to Main Page]][/b][/f]

227

251

228

252

229

253

!Aragats Solar Neutron Telescope (ASNT)

230

[b]A[/b]ragats [b]S[/b]olar [b]N[/b]eutron [b]T[/b]elescope ([b]ASNT[/b]) located on the slope of the mountain Aragats (Armenia, 40.47N, 44.18E, 3200m above sea leve). ASNT is

254

[b]A[/b]ragats [b]S[/b]olar [b]N[/b]eutron [b]T[/b]elescope ([b]ASNT[/b]) located on the slope of the mountain Aragats (Armenia, 40.47N, 44.18E, 3200m above sea level). ASNT is

231

255

formed from 4 separate identical modules, as shown in Figure 1. Each module consists of standard slabs of 50x50x5cm^3 plastic scintillators stacked vertically on 2 layer

232

256

of 4 50x50x5cm^3 horizontal plastic scintillator slabs. Scintillator slabs are fine polished to provide good optical contact of the assembly. The slab assembly (scintillator

233

257

housing) is covered by white paper from the sides and bottom and firmly kept together with special belts. Total thickness of the assembly is 60cm. Four detectors of

234

258

100x100x5cm^3 size each located above the thick scintillator assembly as is seen in Figure 1, are used to indicate if charged particle traverse near vertically. This

235

259

information is used for selecting neutral particles and “vetoing” charged particles. A scintillator light capture cones and Photo Multiplier Tubes (large cathode, FEU 49 type)

236

are located on the top of scintillator housing in special iron shielding, where as well the high voltage power supply and preamplifiere are located.

260

are located on the top of scintillator housing in special iron shielding, where as well the high voltage power supply and preamplifiers are located.

237

261

238

262

{| border="1px"

239

263

[url="setups/asec/pictures/678px-ASNT.jpg"][img]setups/asec/pictures/300px-ASNT.jpg[/img][/url]

269

293

270

294

271

295

272

273

274

275

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

276

[f] [[Main Page]][/f]

296

297

298

299

300

[f] [b][[Main Page|Return to Main Page]][/b][/f]

277

301

</page>

278

279

280

281

282

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

283

[f] [[Main Page]][/f]

284

285

286

!Electric Field Monitor Boltek EFM100 Aragats

287

302

303

304

305

306

[f] [b][[Main Page|Return to Main Page]][/b][/f]

307

308

309

!Electric Field Monitor Boltek EFM-100

310

311

Measuring the Boltek EFM-100 not only detects nearby lightning but can detect the atmospheric

312

conditions which precede lightning.

313

314

315

Boltek EFM-100 Electric Field Monitor measures the static electric field generated by

316

thunderclouds electric field in Volts per meter (measurement accuracy 5%.). Lightning is

317

detected as a sudden change in the static electric field.

318

319

320

The electric charge contained in a thundercloud also generates an electric field. This

321

field can be measured on the ground.

322

323

324

EFM-100 can

325

*Log date, time and distance of nearby lightning.

326

*Monitor lightning up to 38 km away.

327

*Detect the high electric field conditions which precede lightning.

328

*Short-range detector is optimized for close lightning to provide the best distance accuracy while ignoring far away lightning.

329

*Monitor up to four separate locations per PC.

330

*Watch trends develop.

331

*Attention getting alarms.

332

*Review archived data from previous storms.

333

*Stay current with free software updates from the Boltek website.

334

335

More information about the Boltek EFM-100 can be found at the [url="http://www.boltek.com/efm100.html"]manufacturer's website[/url]. [br]

288

336

289

337

{| border="1px"

290

338

[url="setups/asec/pictures/800px-BoltekEFM-100_Yerevan.JPG"][img]setups/asec/pictures/300px-BoltekEFM-100_Yerevan.JPG[/img][/url]

291

339

292

[i][b]Figure 1:[/b] Electric Field Monitor Boltek EFM100.[/i]

340

[i][b]Figure 1:[/b] Electric Field Monitor Boltek EFM-100[/i]

293

341

294

342

295

Text

296

297

298

299

300

301

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

302

[f] [[Main Page]][/f]

343

344

345

346

347

348

[f] [b][[Main Page|Return to Main Page]][/b][/f]

303

349

</page>

304

305

306

307

308

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

309

[f] [[Main Page]][/f]

310

311

312

!Lightning Detector Boltek LD Aragats

313

314

350

351

352

353

354

[f] [b][[Main Page|Return to Main Page]][/b][/f]

355

356

357

!Lightning Detector Boltek StormTracker

358

359

Boltek’s StormTracker Lightning Detection System, powered by the software from Astrogenic systems,

360

deﬁne four types of lightning occurrences (CG- , CG+ cloud-to ground negative and positive, IC - ,

361

IC+ intracloud positive and negative, - in radii of 1, 3, 5 and 10 km around the location of its antenna).

362

363

364

StormTracker's antenna is a small black box (3"x2"x1-1/2") which may be mounted indoors or outdoors. The

365

antenna is typically mounted ten to twenty feet above the ground, away from large metal objects and

366

sources of electrical noise such as televisions and computer monitors.

367

368

369

StormTracker's

370

*Detects if lightning is near.

371

*Receives early warning of approaching or developing storms.

372

*Configurable Severe Storm and Close Storm Alarms.

373

*Determines from which direction the approaching storm is coming.

374

*Follows developing and decaying storms from the first strike to the last.

375

*Saves all data for future analysis.

376

377

StormTracker works by detecting the radio signals produced by lightning. These are the same signals

378

you can hear on an AM radio during a thunderstorm. StormTracker's direction-finding antenna provides

379

direction information while storm distance is calculated from received signal strength. Special

380

processing in software reduces the effects of strike-to-strike energy variations providing more

381

accurate distance information.

382

383

384

More information about the Boltek StormTracker can be found at the [url="http://www.boltek.com/stormtracker.html"]manufacturer's website[/url]. [br]

315

385

{| border="1px"

316

[url="setups/asec/pictures/Anthand-t.jpg"][img]setups/asec/pictures/100px-Anthand-t.jpg[/img][/url]

386

[url="setups/asec/pictures/PCIBoardAntenna92-StormTracker.png"][img]setups/asec/pictures/PCIBoardAntenna92-StormTracker.png[/img][/url]

317

387

318

[i][b]Figure 1:[/b] Lightning Detector Boltek LD250.[/i]

388

[i][b]Figure 1:[/b] Lightning Detector Boltek StormTracker.[/i]

319

389

320

390

321

Page Under Construction.

322

323

324

325

326

327

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

328

[f] [[Main Page]][/f]

391

392

393

394

395

396

[f] [b][[Main Page|Return to Main Page]][/b][/f]

329

397

</page>

330

331

332

333

334

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

335

[f] [[Main Page]][/f]

398

399

400

401

402

[f] [b][[Main Page|Return to Main Page]][/b][/f]

336

403

337

404

338

405

!Cube

339

406

407

The Cube assembly (Figure 1) consists of two 20-cm thick scintillators of 0.25-m^2 area each,

408

enfolded by 1-cm thick, 1-m^2 area scintillators. This design ensures that no particle may hit

409

the inside 20 cm without hitting the surrounding ‘‘veto’’ scintillators. The 20-cm thick plastic

410

scintillators are overviewed by the photomultiplier PM-49 with a large cathode operating in a

411

low-noise regime. Surrounding detectors (six units) are 1-cm thick molded plastic scintillators.

412

The efﬁciency of neutral component detection by 1-cm thick scintillators is ~2% and weakly

413

depends on the energy of gamma rays. The energy losses of passing electrons and muons in

414

20-cm-thick plastic scintillator are ~40 MeV. Taking into account the construction material

415

of the detector (2-mm iron tilt and 1-cm plastic scintillator), and the roof of the building

416

(1-mm iron tilt), the electron registration energy threshold for the upper 20-cm-thick scintillator

417

is estimated to be about 8 MeV and the bottom one ~40 MeV for the vertical ﬂux. The obtained

418

efﬁciency of gamma ray registration equals ~20% and weakly depends on energy.

419

420

421

Efficiency of neutron detection in the range 4-100 MeV, in 20 cm thick scintillator is ~27%. CUBE

422

assembly has been tested in Yerevan at 1000 m. a.s.l. and in 2010 installed at high altitude

423

“Aragats” research station (3200 m a.s.l.). It has been included into Aragats Space Environmental

424

Center (ASEC) since September 15, 2010; the on-line time series are available from the CRD portal: [url="http://adei.crd.yerphi.am/adei/"]http://adei.crd.yerphi.am/adei/[/url]

425

426

427

More description of the Cube detector can be found in [url="http://dx.doi.org/10.1016/j.atmosres.2012.05.008"]A. Chilingarian et al. Atmospheric Research 114–115 (2012)[/url] [br]

428

340

429

{| border="1px"

341

430

[url="setups/asec/pictures/cube.jpg"][img]setups/asec/pictures/300px-cube.jpg[/img][/url]

342

431

343

432

[i][b]Figure 1:[/b] Cube Monitor.[/i]

344

433

345

434

346

Page Under Construction

347

348

349

350

351

352

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

353

[f] [[Main Page]][/f]

435

436

437

438

439

440

[f] [b][[Main Page|Return to Main Page]][/b][/f]

354

441

</page>

355

356

357

358

359

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

360

[f] [[Main Page]][/f]

361

362

363

!Magnetotelluric Station (MTS) Lemi-417

364

442

443

444

445

446

[f] [b][[Main Page|Return to Main Page]][/b][/f]

447

448

449

!Magnetotelluric Station (MTS) LEMI-417

450

451

This page is under construction; however, information about the Lemi Magnetotelluric Station can be found at the [url="http://www.isr.lviv.ua/lemi417.htm"]manufacturer's website[/url].

365

452

366

453

{| border="1px"

367

454

[url="setups/asec/pictures/LEMI-417.jpg"][img]setups/asec/pictures/LEMI-417.jpg[/img][/url]

368

455

369

[i][b]Figure 1:[/b] Magnetotelluric Station (MTS) Lemi-417.[/i]

456

[i][b]Figure 1:[/b] Magnetotelluric Station (MTS) LEMI-417.[/i]

370

457

371

458

372

459

Page Under Construction.

373

460

374

461

375

376

377

378

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

379

[f] [[Main Page]][/f]

462

463

464

465

466

[f] [b][[Main Page|Return to Main Page]][/b][/f]

380

467

</page>

381

382

383

384

385

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

386

[f] [[Main Page]][/f]

468

469

470

471

472

[f] [b][[Main Page|Return to Main Page]][/b][/f]

387

473

388

474

389

475

!MAKET-ANI Extensive Air Shower Detector

397

483

[i][b]Figure 1:[/b] MAKET-ANI Extensive Air Shower Detector.[/i]

398

484

399

485

400

After obtaining and publishing final results of the MAKET-ANI (see Figure 10) experiment (Chilingarian, et al., 2007) the experiment was stopped for collecting high energy galactic cosmic rays. Some of the scintillators were used for rearranged smaller detector. Around the ASNT detector (consisted of four 60 cm thick scintillators and four 5 cm thick scintillators another 8 5 cm scintillators were arranged and attached to the 16 channel spectrum analyzer. We plan to test with this array new fast-timing technique to be used for new big array in Nor Amberd (Chilingarian, Hovsepyan, et al, 2007). Meanwhile new MAKET array provides following information:

486

After obtaining and publishing final results of the MAKET-ANI (see Figure 10) experiment (Chilingarian, et al., 2007) the experiment was stopped for collecting high energy galactic cosmic rays. Some of the scintillators were used for rearranged smaller detector. Around the ASNT detector (consisted of four 60 cm thick scintillators and four 5 cm thick scintillators another 8 5 cm scintillators were arranged and attached to the 16 channel spectrum analyzer. We plan to test with this array new fast-timing technique to be used for new big array in Nor-Amberd (Chilingarian, Hovsepyan, et al, 2007). Meanwhile new MAKET array provides following information:

401

487

402

488

*1 minute count rates of all 16 channels of the MAKET (see Table 19);

403

489

*Count rate of the EAS triggering 8 and all 16 detectors;

405

491

*16 x 16 correlation matrix of MAKET channels calculated by five-second count rates in 1 minute.

406

492

407

493

408

In the directory “DEFOULT” following information is stored:

494

In the directory “DEFAULT” following information is stored:

409

495

410

496

*Columns 1-16 - the count rates of all 16 MAKET channels: first 4 columns – from 60 cm scintillators, 5-16 columns – from 5 cm scintillator. The count rates are posted in the Table 19;

411

497

*Columns 17-18 – the count rates corresponding to the EAS initiated triggers. 17th column corresponds to the coincidence of the first 8 channels (ASNT scintillators), 18th column corresponding to the coincidence in all 16 channels. The count rates are posted in the Table 20;

422

508

*In the files with “events” extension is related to the Extensive Air Showers (EAS). The logical software trigger selects events when signals are more than in 8 detectors.

423

509

424

510

425

426

427

428

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

429

[f] [[Main Page]][/f]

511

512

513

514

515

[f] [b][[Main Page|Return to Main Page]][/b][/f]

430

516

</page>

431

432

433

434

435

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

436

[f] [[Main Page]][/f]

517

518

519

520

521

[f] [b][[Main Page|Return to Main Page]][/b][/f]

437

522

438

523

439

524

!NaI(Tl) Monitor

440

525

441

442

Page Under Construction.

526

The NaI network is located in the same experimental hall as the Cube detector; it consists of ﬁve

527

NaI crystal scintillators in the sealed aluminum (1-mm-thick) housing. The NaI crystal is surrounded

528

by 0.5 cm of magnesium by all sides (because the crystal is hygroscopic) with a transparent window

529

directed to the photo-cathode of the photomultiplier tube PM-49. The large cathode of PM-49 (15-cm

530

diameter) provides good light collection. The spectral sensitivity range of PM-49 is 300–850 nm, which

531

covers the spectrum of NaI(Tl) emission light. The sensitive area of each NaI crystal is ~0.032 m2;

532

the total area of the ﬁve crystals is ~0.16 m^2; the efﬁciency to detect gamma rays is ~80%.

533

534

535

For the channels of 3–4 MeV, NaI crystals underestimate the intensity due to lower efﬁciency of gamma

536

ray detection near the electronic threshold. For the highest energies (above 60 MeV), gamma rays may

537

not deposit their whole energy in the crystal.

538

539

540

More information about the NaI Detector network can be found in [url="http://dx.doi.org/10.1088/1742-6596/409/1/012218"]Avakyan et al. (2013)[/url].

443

541

444

542

445

543

{| border="1px"

446

[url="setups/asec/pictures/800px-MAKET_ANI.jpg"][img]setups/asec/pictures/400px-MAKET_ANI.jpg[/img][/url]

544

[url="http://crd.yerphi.am/files/Monitors/Figures/big/NAI.jpg"][img]http://crd.yerphi.am/files/Monitors/Figures/big/NAI.jpg[/img][/url]

447

545

448

[i][b]Figure 1:[/b] MAKET-ANI Extensive Air Shower Detector.[/i]

546

[i][b]Figure 1:[/b] NaI scintillator detector.[/i]

449

547

450

548

451

549

452

453

454

455

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

456

[f] [[Main Page]][/f]

550

551

552

553

554

[f] [b][[Main Page|Return to Main Page]][/b][/f]

457

555

</page>

458

459

460

461

462

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

463

[f] [[Main Page]][/f]

464

465

466

!Basic detecting unit of the SEVAN network at Aragats

467

468

The basic detecting unit of the SEVAN network (see Figure 11) is assembled from standard slabs of 50x50x5cm plastic scintillators. Between 2 identical assemblies of 100x100x5m scintillators (four standard slabs) are located two 100x100x5cm lead absorbers and thick 50x50x25cm scintillator assembly (5 standard slabs). A scintillator light capture cone and [b]P[/b]hoto [b]M[/b]ultiplier [b]T[/b]ube ([b]PMT[/b]) are located on the top, bottom and the intermediate layers of detector. The detailed detector charts with all sizes are available from http://192.168.24.118/.

556

557

558

559

560

[f] [b][[Main Page|Return to Main Page]][/b][/f]

561

562

563

!Basic detecting unit of the SEVAN ([u]S[/u]pace [u]E[/u]nvironmental [u]V[/u]iewing and [u]A[/u]nalysis [u]N[/u]etwork)

564

565

The basic detecting unit of the SEVAN network (see Figure 1) is assembled from standard slabs of

566

50x50x5cm plastic scintillators. Between 2 identical assemblies of 100x100x5m scintillators (four

567

standard slabs) are located two 100x100x5cm lead absorbers and thick 50x50x25cm scintillator assembly

568

(5 standard slabs). A scintillator light capture cone and [b]P[/b]hoto [b]M[/b]ultiplier [b]T[/b]ube

569

([b]PMT[/b]) are located on the top, bottom and the intermediate layers of detector.

469

570

470

571

471

572

{| border="1px"

474

575

[i][b]Figure 1:[/b] The basic detecting unit of the SEVAN network.[/i]

475

576

476

577

477

At the Nor-Amberd research station of ASEC we are starting tests of the operation of the SEVAN detector prototype (SEVAN #1) with slightly reduced sizes: area of upper and lower 5cm this scintillators are 0.65m, instead of 1m, and thickness of middle detector is 20cm, instead of 25cm. Also we establish the SEVAN detector prototype (SEVAN #2) in the Yerevan and in the Aragats (SEVAN #3). The dimensions of the upper and lower scintillaors are 1m, and thickness of middle detector is 20cm.

478

479

Incoming neutral particles undergo nuclear reactions in the thick 25cm plastic scintillator and produce protons and other charged particles. In the upper 5cm thick scintillator charged particles are registered very effectively; however for the nuclear interactions of neutral particles there is not enough substance. When a neutral particle traverses the top thin (5cm) scintillator, usually no signal is produced. The absence of the signal in the upper scintillators, coinciding with the signal in the middle scintillator, points to neutral particle detection. The coincidence of signals from the top and bottom scintillators indicates traversal of high energy muons. Lead absorbers improve efficiency of the neutral flux detection and filtered low energy charged particles. SEVAN world-wide network will consist of modules located in Croatia, Bulgaria, India (to be installe din 2008), Slovakia, Costa-Rica and Indonesia (to be installed in 2009). We present data from SEVAN module operated at Nor Amberd research station, another module is under construction in Yerevan at altitude 1000m in CRD headquarters

480

578

At the Nor-Amberd research station of ASEC we are starting tests of the operation of

579

the SEVAN detector prototype (SEVAN #1) with slightly reduced sizes: area of upper and

580

lower 5cm this scintillators are 0.65m, instead of 1m, and thickness of middle detector

581

is 20cm, instead of 25cm. Also we establish the SEVAN detector prototype (SEVAN #2) in

582

the Yerevan and in the Aragats (SEVAN #3). The dimensions of the upper and lower

583

scintillators are 1m, and thickness of middle detector is 20cm.

584

585

586

Incoming neutral particles undergo nuclear reactions in the thick 25cm plastic scintillator

587

and produce protons and other charged particles. In the upper 5cm thick scintillator charged

588

particles are registered very effectively; however for the nuclear interactions of neutral

589

particles there is not enough substance. When a neutral particle traverses the top thin (5cm)

590

scintillator, usually no signal is produced. The absence of the signal in the upper scintillators,

591

coinciding with the signal in the middle scintillator, points to neutral particle detection. The

592

coincidence of signals from the top and bottom scintillators indicates traversal of high energy

593

muons. Lead absorbers improve efficiency of the neutral flux detection and filtered low energy

594

charged particles. SEVAN world-wide network will consist of modules located in Croatia, Bulgaria,

595

India (to be installed in 2008), Slovakia, Costa-Rica and Indonesia (to be installed in 2009). We

596

present data from SEVAN module operated at Nor-Amberd research station, another module is under

597

construction in Yerevan at altitude 1000m in CRD headquarters

481

598

!!Structure of the information content from SEVAN detector

482

599

483

600

The following information is providing by SEVAN detector:

484

601

485

*Count rates from the all 3 layers (see Table 16).

486

*Count rates of the all coincidences of upper, middle and lower detectors (see Table 16 and Table 17).

487

*Correlation matrix between all detected signals (Table 18)

488

489

In the directory “DEFAULT” the following information is stored:

490

491

*columns 1-3 - the count rates of all channels of the SEVAN. The count rates are posted in the Table 16;

492

*column 4 unused (this channel we can use as input of the atmospheric pressure sensor).

493

*columns 5-8 – the count rates of the coincidences of the all channels of the SEVAN. If we denote by the sign “1” signal from scintillator, and by sign “0” absence of signal, following combinations of the 3-layered detector output are stored: 110, 101, 011, 111 (see Table 16).

494

495

496

497

498

499

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

500

[f] [[Main Page]][/f]

602

*Count rates from the all 3 layers.

603

*Count rates of the all coincidences of upper, middle and lower detectors.

604

*Correlation matrix between all detected signals.

605

606

607

608

609

610

611

[f] [b][[Main Page|Return to Main Page]][/b][/f]

501

612

</page>

502

503

504

505

506

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

507

[f] [[Main Page]][/f]

508

509

510

!Stand

511

512

Stand is assembled from standard slabs of 50x50x5cm plastic scintillators. Between 2 identical assemblies of 100x100x5m scintillators (four standard slabs) are located two 100x100x5cm lead absorbers and thick 50x50x25cm scintillator assembly (5 standard slabs). A scintillator light capture cone and [b]P[/b]hoto [b]M[/b]ultiplier [b]T[/b]ube ([b]PMT[/b]) are located on the top, bottom and the intermediate layers of detector. The detailed detector charts with all sizes are available from http://192.168.24.118/.

613

614

615

616

617

[f] [b][[Main Page|Return to Main Page]][/b][/f]

618

619

620

!Stand 1cm

621

622

Stand 1cm detector comprise of three-layer assembly of 1 cm thick 1 m^2 sensitive area molded plastic

623

scintillators one above the other and one 3 cm thick scintillator located aside (Figure 1).

624

625

626

Detector operates in particle counter regime. Outdoors location, 1-cm thickness and three-layer design

627

allow to measure flux of TGE electrons with 3 different energy thresholds starting from 1.5 MeV and to

628

recover integral spectrum of TGE electrons.

629

630

631

Light from scintillator by optical spectrum-shifter ﬁbers is reradiated to the long wavelength region

632

and passed to the photomultiplier FEU-115M type photomultiplier (PM). The maximum of luminescence is

633

emitted at a 420-nm wavelength and the luminescence time is about 2.3 ns. The tuning of the Stand 1cm

634

detector consists in selections of PM high voltage and discrimination thresholds. The threshold should

635

be chosen to guarantee both high efﬁciency of signal detection and maximal suppression of PM noise.

636

Proper tuning of the detector provides ~99% efﬁciency of charged particle detection. The data acquisition

637

system counts and stores all coincidences of the detector channels.

638

639

640

Coincidence ‘‘100’’ means that only the upper detector registers a particle. This combination registered

641

low energy electrons with an efﬁciency of ~99% (we assume that the efﬁciency of electron registration

642

in the second scintillator also is 99%). We estimate the minimal energy of an electron stopping in the

643

upper detector and giving a signal to be ~1.4 MeV; it is the lowest energy threshold among all ASEC

644

detectors. Gamma ray detecting efﬁciency of this combination is about 2%. For the coincidence 010,

645

the gamma ray detection efﬁciency is increased to ~3% due to creation of electron-positron pairs in the

646

substance of the upper scintillator. Coincidence ‘‘111’’ means that all three layers register particles;

647

the minimal energy of charged particles giving a signal in all three layers is ~12 MeV. The energy

648

threshold of 3cm thick scintillators is ~5MeV.

513

649

514

650

515

651

{| border="1px"

516

652

[url="setups/asec/pictures/stand.jpg"][img]setups/asec/pictures/300px-stand.jpg[/img][/url]

517

653

518

654

[i][b]Figure 1:[/b] Stand Monitor.[/i]

519

655

520

656

521

522

523

524

525

!!Structure of the information content from SEVAN detector

526

527

The following information is providing by SEVAN detector:

528

529

*Count rates from the all 3 layers (see Table 16).

530

*Count rates of the all coincidences of upper, middle and lower detectors (see Table 16 and Table 17).

531

*Correlation matrix between all detected signals (Table 18)

532

533

In the directory “DEFAULT” the following information is stored:

534

535

*columns 1-3 - the count rates of all channels of the SEVAN. The count rates are posted in the Table 16;

536

*column 4 unused (this channel we can use as input of the atmospheric pressure sensor).

537

538

539

540

541

542

543

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

544

[f] [[Main Page]][/f]

657

658

659

660

661

662

[f] [b][[Main Page|Return to Main Page]][/b][/f]

545

663

</page>

546

547

548

549

550

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

551

[f] [[Main Page]][/f]

664

665

666

667

668

[f] [b][[Main Page|Return to Main Page]][/b][/f]

552

669

553

670

554

671

!Stand_3cm

555

672

556

557

Page under construction.

558

559

560

561

562

563

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

564

[f] [[Main Page]][/f]

565

</page>

566

567

568

569

570

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

571

[f] [[Main Page]][/f]

572

573

574

!Vantage Pro 2 Weather Station

575

576

577

Page Under Construction.

578

579

580

581

582

583

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

584

[f] [[Main Page]][/f]

585

</page>

586

587

588

589

590

591

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

592

[f] [[Main Page]][/f]

593

594

595

!About NorAmberd Research Station

596

597

{| border="1px"

598

[url="setups/asec/pictures/AragatsStation2009.jpg"][img]setups/asec/pictures/1200px-AragatsStation2009.jpg[/img][/url]

599

600

[i][b]Figure 1:[/b] Aragats Station, altitude 3200m above sea level.[/i]

601

602

603

Page Under Construction.

604

605

Cosmic Ray research at high altitude stations on Mt. Aragats, Armenia, was founded by famous Armenian physicists, Alikhanyan brothers, in 1943. Research facilities are located on

606

two high-altitude stations on Mt.Aragats, Nor-Amberd (40.37N, 44.26E, 2000m above sea level) Station and Aragats Station (40.47N, 44.18E, 3200m above sea level), and at CRD

607

headquarters at A.I. Alikhanyan National Science Laboratory, Yerevan.

608

609

610

611

612

613

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

614

[f] [[Main Page]][/f]

615

</page>

616

617

618

619

620

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

621

[f] [[Main Page]][/f]

622

623

624

!NorAmberd Multidirectional Muon Monitor (NAMMM)

625

626

Page Under Construction.

627

628

629

{| border="1px"

630

[url="setups/asec/pictures/612px-AMMM.jpg"][img]setups/asec/pictures/350px-AMMM.jpg[/img][/url] ||

631

[url="setups/asec/pictures/AMMM_fig2.png"][img]setups/asec/pictures/350px-AMMM_fig2.png[/img][/url]

632

633

[i][b]Figure 1:[/b]Aragats Multidirectional Muon Monitor (AMMM).[/i] ||

634

[i][b]Figure 2:[/b]Projection of the AMMM on the X-Y plane.[/i]

635

636

637

638

639

640

641

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

642

[f] [[Main Page]][/f]

643

</page>

644

645

646

647

648

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

649

[f] [[Main Page]][/f]

650

651

652

!NorAmberd Neutron Monitor (NANM)

653

654

Page Under Construction.

655

656

[b]Ar[/b]agats [b]N[/b]eutron [b]M[/b]onitor ([b]ArNM[/b]) in operation at Aragats Station (40.47N, 44.18E, 3200m above sea level) since 2000 year. Neutron Monitore consist

673

“Stand 3cm” detector comprise of four-layer assembly of 3 cm thick 1 m2 sensitive area molded plastic

674

scintillators one above the other.

675

676

677

Tuning of Stand 3cm was made by means of the 8-channel signal analyzer developed at ASEC for online

678

data processing. Proper tuning of the detector provides 98–99% signal detection efﬁciency simultaneously

679

suppressing electronic noise down to 1–2%. The data acquisition (DAQ) electronics measures and stores

680

all coincidences of the signal appearance in the detector channels. Coincidence ‘’1000’’ corresponds

681

to signal registration only from upper scintillator, ‘‘1100’’ – from the ﬁrst two upper scintillators,

682

and so on. GEANT4 simulations demonstrate that Stand 3cm detector can measure count rate of incident

683

electrons with energy thresholds 5, 15, 25, 35 MeV (combinations ‘‘1000’’, ‘‘1100’’, ‘‘1110’’ and ‘‘1111’’).

684

The 5 MeV electrons can give signal above the discrimination level only in the upper scintillator, to be

685

absorbed then in the scintillator body, or in the metallic tilts of scintillator housing; the 15 MeV

686

electrons can penetrate and be registered also in the second scintillator, and so on. In this way,

687

measuring the enhancements of count rates of above mentioned 4 combinations of detector layer operation

688

we can recover the integral energy spectra of TGE electrons, of course, after subtracting the gamma ray

689

contamination.

690

691

692

The electronics signal threshold of Stand 3cm detector is ~3 MeV, thus, all 4 Stand 3cm layers can detect

693

gamma rays with energies greater than ~3 MeV, although with much smaller registration efﬁciencies comparing

694

with electron detection efﬁciencies. Gamma rays should have high enough energy to create high- energy

695

charged particles, which can reach bottom layer (the gamma ray energy should be above 40 MeV to generate

696

signal in all 4 layers with probability 1%).

697

698

699

{| border="1px"

700

[url="setups/asec/pictures/STAND_3cm.jpg"][img]setups/asec/pictures/300px_STAND_3cm.jpg[/img][/url]

701

702

[i][b]Figure 1:[/b] Stand Monitor.[/i]

703

704

705

706

707

708

709

710

[f] [b][[Main Page|Return to Main Page]][/b][/f]

711

</page>

712

713

714

715

716

[f] [b][[Main Page|Return to Main Page]][/b][/f]

717

718

719

!Davis Wireless Vantage Pro2 Plus

720

721

{| border="1px"

722

[url="setups/asec/pictures/WeatherStation1.JPG"][img]setups/asec/pictures/WeatherStation1_small.JPG[/img][/url]

723

724

[i][b]Figure 1:[/b] Weather Station at Aragats.[/i]

725

726

727

At the [[Aragats Research Station]] ([url="https://maps.google.com/maps?q=40.4715N,44.1815E"]40.47N, 44.18E[/url], 3200m a.s.l.)

728

installed Davis Wireless Vantage Pro2 Plus Weather Station (including UV and Solar Radiation Sensors).

729

This Weather Station has the following integrated Sensors:

730

*Rain collector

731

*Temperature and humidity sensors

732

*Anemometer

733

*Solar radiation sensor

734

*UV sensor

735

*Solar panel

736

At the [[Nor-Amberd Research Station]] ([url="https://maps.google.com/maps?q=40.375N,44.2642E"]40.37N, 44.26E[/url], 2000m a.s.l.) and

737

[[Yerevan CRD headquarters]] ([url="https://maps.google.com/maps?q=40.2046N,44.4857E"]40.205N, 44.486E[/url], 1090m a.s.l.)

738

installed Davis Wireless Vantage Pro2 Plus Weather Stations (including 24-Hr Fan Aspirated Radiation Shield).

739

These Weather Stations has the following integrated Sensors:

740

*Rain collector

741

*Temperature and humidity sensors enclosed in our solar-powered, 24-hour fan-aspirated radiation shield (combines active and passive aspiration to minimize the effects of radiation)

742

*Anemometer

743

*Solar radiation sensor

744

*UV sensor

745

*Solar panel

746

747

748

Data of the ASEC Weather Stations updated each hour and available from our Online Data Base named

749

[b]ADEI of ASEC[/b] ([b]A[/b]dvanced [b]D[/b]ata [b]E[/b]xtraction [b]I[/b]nfrastructure of [b]A[/b]ragats [b]S[/b]pace [b]E[/b]nvironmental [b]C[/b]enter).

750

751

752

Description of the measured parameters by the Davis Wireless Vantage Pro2 Plus:

753

754

755

[b]OUTSIDE AIR TEMPERATURE[/b]

756

757

The Davis Vantage Pro Plus uses the Integrated Sensor Suite's temperature sensor to measure the outside air temperature. A second temperature sensor in the console measures the inside air temperature.

758

759

760

[b]HUMIDITY[/b]

761

762

Humidity itself simply refers to the amount of water vapor in the air. However, the amount of water vapor that the air can contain varies with air temperature and pressure. Relative humidity takes into account these factors and offers a humidity reading which reflects the amount of water vapor in the air as a percentage of the amount the air is capable of holding. Relative humidity, therefore, is not actually a measure of the amount of water vapor in the air, but a ratio of the air's water vapor content to its capacity. It is important to realize that relative humidity changes with temperature, pressure, and water vapor content. For a parcel of air with a capacity for 10 g of water vapor, which contains 4 g of water vapor, the relative humidity would be 40%. Adding 2 g more water vapor (for a total of 6 g) would change the humidity to 60%. If that same parcel of air is then warmed so that it has a capacity for 20 g of water vapor, the relative humidity drops to 30% even though the water vapor content does not change.

763

764

Relative humidity is an important factor in determining the amount of evaporation from plants and wet surfaces, since warm air with low humidity has a large capacity for extra water vapor.

765

766

767

[b]DEW-POINT[/b]

768

769

Dew-point is the temperature to which air must be cooled for saturation (100% relative humidity) to occur, providing there is no change in water content. The dew-point is an important measurement used to predict the formation of dew, frost and fog. If dew-point and temperature are close together in the late afternoon when the air begins to turn colder, fog is likely during the night. Dew-point is also a good indicator of the air's actual water vapor content, unlike relative humidity, which also takes the air's temperature into account. High dew-point indicates high vapor content, low dew-point indicates low vapor content. In addition a high dew-point indicates a better chance of rain and severe thunderstorms. You can even use dew-point to predict the minimum overnight temperature. Providing no new fronts are expected overnight and the afternoon relative humidity is more than 50%, the afternoon's dew point gives you an idea of what minimum temperature to expect overnight, since the air is not likely to get colder than the dew-point anytime during the night.

770

771

772

[b]Wind[/b]

773

774

Air that flows in relation to the earth's surface, generally horizontally. There are four areas of wind that could be measured: direction, speed, character (gusts and squalls), and shifts. Surface winds are measured by wind vanes and anemometers, while upper level winds are detected through pilot balloons, rawin, or aircraft reports.

775

776

The weather station measures direction, speed and gusts speed. Its anemometer is located two meters above the rooftop of the house.

777

778

779

[b]Wind speed[/b]

780

781

The wind speed is measured with a so-called anemometer and is determined by counting rotation pulses over a sample period. The sample period is 2.25 seconds. The number of pulses per sample period is equal to the wind speed in miles per hour. In the database the wind speed is expressed in km/hr. The conversion factor for some frequently used units is as follows: 1 MPH = 1.6093 kph = 0.4470 m/sec = 0.8690 knots. The conversion to the well-known Beaufort scale is less obvious.

782

783

784

[b]Wind direction[/b]

785

786

The direction from which the wind is blowing. For example, an easterly wind is blowing from the east, not toward the east. It is reported with reference to true north, or 360 degrees on the compass, and expressed to the nearest 10 degrees, or to one of the 16 points of the compass (N, NE, WNW, etc.).

787

788

789

[i]From North[/i]

790

{| border="1px"

791

North [br]

792

North-Northeast [br]

793

Northeast [br]

794

East-Northeast [br]

795

East [br]

796

East-Southeast [br]

797

Southeast [br]

798

South-Southeast [br]

799

800

0°or360°[br]

801

22.5° [br]

802

45° [br]

803

67.5° [br]

804

90° [br]

805

112.5° [br]

806

135° [br]

807

157.5° [br]

808

809

South [br]

810

South-Southwest [br]

811

Southwest [br]

812

West-Southwest [br]

813

West [br]

814

West-Northwest [br]

815

Northwest [br]

816

North-Northwest [br]

817

818

180° [br]

819

202.5° [br]

820

225° [br]

821

247.5° [br]

822

270° [br]

823

292.5° [br]

824

315° [br]

825

337.5° [br]

826

827

828

829

[b]Wind run[/b]

830

831

Wind run is a measure of the amount of wind which passes a given point during the measurement period. To calculate wind run, multiply the speed by the length of time in the measurement period. For example 10 km/hr for 12 hours would be 120 kilometers of wind run. Since the basic measuring period of the present weather station is one hour, the wind run is equal to the wind speed.

832

833

834

[b]Wind Chill[/b]

835

836

Wind Chill takes into account how the speed of the wind affects our perception of air temperature. Our bodies warm the surrounding air molecules by transferring heat from the skin. If there is no air movement, this insulating layer of warm air molecules stays next to the body and offers some protection from cooler air molecules. However, wind sweeps that comfy warm air surrounding the body away. The faster the wind blows, the faster the heat is carried away and the cooler you feel. Above 91° F, wind movement has no effect on the apparent temperature, so wind chill is the same as the outside temperature.

837

838

839

[b]Heat Index[/b]

840

841

Heat Index uses the temperature and the relative humidity to determine how hot the air actually 'feels'. When humidity is low, the apparent temperature will be lower than the air temperature, since perspiration evaporates rapidly to cool the body. However, when humidity is high (i.e., the air is saturated with water vapor) the apparent temperature 'feels' higher than the actual air temperature, because perspiration evaporates more slowly. The heat index is only measured when the air temperature is above 14° c because it is insignificant at lower air temperatures. (Below 14° c, heat index = air temperature). The heat index is not calculated above 52° c.

842

843

844

[b]THW (Temperature - Humidity - Wind) Index[/b]

845

846

THW Index uses humidity and temperature to calculate an apparent temperature.

847

848

849

[b]THSW (Temperature - Humidity - Sun - Wind) Index[/b]

850

851

THSW Index uses humidity and temperature to calculate an apparent temperature. In addition, THSW incorporates the heating effects of direct solar radiation and the cooling effects of wind on our perception of temperature.

852

853

854

[b]BAROMETRIC PRESSURE[/b]

855

856

The weight of the air that makes up our atmosphere exerts a pressure on the surface of the earth. This pressure is known as atmospheric pressure. Generally, the more air above an area, the higher the atmospheric pressure, this, in turn, means that atmospheric pressure changes with altitude. For example, atmospheric pressure is greater at sea-level than on a mountain top. To compensate for this difference and facilitate comparison between locations with different altitudes, atmospheric pressure is generally adjusted to the equivalent sea-level pressure. This adjusted pressure is known as barometric pressure. In reality, the Davis Vantage Pro Plus measures atmospheric pressure, but then translates this to barometric pressure.

857

858

Barometric pressure also changes with local weather conditions, making barometric pressure an extremely important and useful weather forecasting tool. High pressure zones are usually associated with fair weather while low pressure zones are generally associated with poor weather. For forecasting purposes, however, the absolute barometric pressure value is generally less important than the change in barometric pressure. In general, rising pressure indicates improving weather conditions while falling pressure indicates deteriorating weather conditions

859

860

861

[b]Rain rate[/b]

862

863

The average amount of rain measured in a time period. The weather station expresses this value in mm's per hour.

864

865

866

[b]Rain[/b]

867

868

The amount of rain measured by the weather station in day time (between sunrise and sunset). The value has no meteorological meaning, but is merely determined to check the holiday weather conditions.

869

870

871

[b]SOLAR RADIATION[/b]

872

873

What we call 'current solar radiation' is technically known as Global Solar Radiation, a measure of the intensity of the sun's radiation reaching a horizontal surface. This irradiance includes both the direct component from the sun and the reflected component from the rest of the sky. The solar radiation reading gives a measure of the amount of solar radiation hitting the solar radiation sensor at any given time, expressed in Watts / sq.m (W/m²).

874

Bright sunshine is considered to be occurring when the solar radiation level exceeds 100 W/m², so we can easily work out how many hours of sunshine occur daily from this reading.

875

876

877

[b]Solar energy[/b]

878

879

The amount of accumulated solar radiation energy over a period of time is measured in Langleys.

880

881

1 Langley = 11.622 Watt-hours per square meter = 3.687 BTUs per square foot = 41.84 kiloJoules per square meter

882

883

884

[b]UV index[/b]

885

886

The UV Index measures the intensity of UV. It uses a scale of 0 to 16 to rate the current intensity of UV. The UV value logged by WeatherLink is the average UV measured during the archive interval. The UV sensor detects Ultraviolet Radiation at wavelengths of 290 to 390 nanometers. The US EPA categorizes the UV Index values as shown below:.

887

*0-2 Minimal

888

*3-4 Low

889

*5-6 Moderate

890

*7-9 High

891

*10+ Very High

892

893

894

[b]COOLING DEGREE DAYS[/b]

895

896

Cooling degree days (CDD) are used to estimate the amount of air conditioning usage during the warm season. To calculate CDDs, you must first find the mean temperature for the day. This is usually done by taking the high and low temperature for the day, adding them together and dividing by two. If the mean temperature is at or below 18.3°C, then the CDD value is zero. If the mean temperature is above 18.3 °C, then the CDD amount equals the mean temperature minus 18.3 °C. For example, if the mean temperature was 25 °C then the CDD amount equals 6.7 °C.

897

898

We will not get a reading during the autumn and winter, unless we get a particularly hot day.

899

900

901

[b]HEATING DEGREE DAYS[/b]

902

903

Heating degree days (HDD) are used to estimate the amount of energy required for residential space heating during the cool season. To calculate the HDDs you must first find the mean temperature for the day. This is usually done by taking the high and low temperature for the day, adding them together and dividing by two. If the mean temperature is at or above 18.3 °C, then the HDD amount is zero. If the mean temperature is below 18.3 °C, then the HDD amount equals 18.3 minus the mean temperature. For example, if the mean temperature was 8.0 °C then the HDD amount equals 10.3 °C.

904

905

We will not get a reading during the spring and summer, unless we get a particularly cold day.

906

907

908

[b]EVAPOTRANSPIRATION (ET)[/b]

909

910

EvapoTranspiration (ET) is a measurement of the amount of water vapor returned to the air in a given area. It combines the amount of water vapor returned through evaporation (from wet vegetation surfaces and the stoma of leaves) with the amount of water vapor returned through transpiration (exhalings of moisture through plant skin) to arrive at a total. Effectively, ETo is the opposite of rainfall, and is expressed in the same units of measure (Inches or millimeters)

911

912

The Davis Vantage Pro Plus uses air temperature, relative humidity, average wind speed, and solar radiation data to estimate ET.

913

914

915

[b]Archive Interval (Arc. Int.)[/b]

916

917

Archive interval is user-selectable time-period from the following intervals (in minutes): 1, 5, 10, 15, 30, 60, or 120.

918

919

920

[b]Reception rate[/b]

921

922

The Reception rate shows the percentage of data packets that have been successfully received by the Vantage Pro console. It is a measure of the reception quality. Values above 90% are normal when the house is not occupied, otherwise the value can be as low as 20%. This is probably caused by interfering transmitters - e.g. notebook computers, or other MHz transmitters.

923

924

The ISS Reception numbers are intended to show the overall quality level of the radio reception between the Vantage Pro consoles and the ISS transmitter. The reception value is a percentage calculated from the number of wind speed samples received (reported in the “Wind Samp” column of the data browser) divided by the expected number of packets. The possible number of wind samples is based upon the transmitter ID and the archive interval period. Since wind speed data is in every data packet, it is possible to determine how many packets should have been received during the archive interval.

925

926

927

Also you can find description of the measured parameters and specification sheets you can find by the folowing links:

928

*[url="http://www.isleofwightweather.co.uk/weather_terms.htm"]Link #1[/url]

929

*[url="http://alaingazon.ca/Meteo/Stationmeteo/glossairestationmeteo.html#Cooling%20degree-days"]Link #2[/url]

930

*[url="setups/asec/pictures/WeatherStationVariables.pdf"]Link #3 (pdf)[/url]

931

*[url="setups/asec/pictures/WeatherStationSpecifications.pdf"]Specification Sheets (pdf)[/url]

932

933

934

935

936

937

938

939

[f] [b][[Main Page|Return to Main Page]][/b][/f]

940

</page>

941

942

943

944

945

[f] [b][[Main Page|Return to Main Page]][/b][/f]

946

947

948

!About Nor-Amberd Research Station

949

950

{| border="1px"

951

(Image of Nor-Amberd Station)

952

953

[i][b]Figure 1:[/b] Nor-Amberd Station, altitude 2000m above sea level.[/i]

954

955

956

The Nor-Amberd Research Station ([url="https://maps.google.com/maps?q=40.375N,44.2642E"]40.37N, 44.26E[/url], 2000m a.s.l.)

957

is the companion to [[Aragats Research Station]] ([url="https://maps.google.com/maps?q=40.4715N,44.1815E"]40.47N, 44.18E[/url], 3200m a.s.l.);

958

both were founded by [url="https://en.wikipedia.org/wiki/Artyom_Alikhanian"]Artyom Alikhanyan[/url] and [url="https://en.wikipedia.org/wiki/Abraham_Alikhanov"]Abraham Alikhanov[/url] in 1943. Located on the slopes of Mt. Aragats, near the village of Byurakan, Armenia, the Nor-Amberd Research Station observes high-energy particles coming from distant galaxies, the Sun, and thunderstorms. [br]

959

960

!Geography and Climate

961

962

Nor-Amberd Research Station is located on Mt. Aragats, a dormant stratovolcano in central Armenia, approximately 30 km (19 mi) northwest of Yerevan, Armenia. The youngest lava flows date between the late-Pleistocene and 3000 BCE (Kharakanian et al., 2003). As such, the station is located on solid volcanic rock foundations. Nor-Amberd Station is 2000m a.s.l., just north of Byurakan Village and near the famous 12th century [url="https://en.wikipedia.org/wiki/Amberd"]Amberd fortress[/url]. [br]

963

964

At the Nor-Amberd Research Station, the average winter temperature is around -3 °C (25 °F), with temperatures occasionally reaching as low as -12 °C (10 °F); during the summer, the average temperature is 15 °C (60 °F), with highs up to 25 °C (80 °F). The average humidity is between 60% and 80%. Average winds are around 10 km/hr (5 mph), with occasional gusts up to 50 km/h (30 mph). [br]

965

966

!Infrastructure

967

968

Nor-Amberd Research Station has facilities housing and maintaing particle detectors for observations of high-energy atmospheric phenomena; networks and servers at Nor-Amberd Research Station collect and store data, as well as forward it to the main campus of the Yerevan Physics Institute. In addition to housing and supporting particle detectors, Nor-Amberd Research station also boasts a fully-fledged conference center, which has a long history of hosting high-energy physics symposia and international forums. Wi-fi networks are available throughout the Nor-Amberd International Conference Center, as well as hotel-like guest rooms.

969

970

971

972

973

974

975

[f] [b][[Main Page|Return to Main Page]][/b][/f]

976

</page>

977

978

979

980

981

[f] [b][[Main Page|Return to Main Page]][/b][/f]

982

983

984

!Nor-Amberd Multidirectional Muon Monitor (NAMMM)

985

986

Page Under Construction.

987

988

989

{| border="1px"

990

image of NAMMM

991

992

[i][b]Figure 1:[/b]Aragats Multidirectional Muon Monitor (AMMM).[/i]

993

994

995

996

997

998

999

1000

[f] [b][[Main Page|Return to Main Page]][/b][/f]

1001

</page>

1002

1003

1004

1005

1006

[f] [b][[Main Page|Return to Main Page]][/b][/f]

1007

1008

1009

!Nor-Amberd Neutron Monitor (NANM)

1010

1011

Page Under Construction.

1012

1013

[b]Ar[/b]agats [b]N[/b]eutron [b]M[/b]onitor ([b]ArNM[/b]) in operation at Aragats Station (40.47N, 44.18E, 3200m above sea level) since 2000 year. Neutron Monitor consist

657

1014

from NM-64 type 18 counter tubes (Moderator: Polyethylene, Reflector: Polyethylene, 3 sections by 6 counters). The monitor is equipped with electronics providing time

658

1015

integration of counts by three dead times. The first dead time equals to 400ns for collecting almost all secondary neutrons generated in the lead of NM. The second dead

659

1016

time is equal to the 0.25ms and the third one equal 1.25ms (as most of NM from world-wide network).

665

1022

666

1023

667

1024

668

669

670

671

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

672

[f] [[Main Page]][/f]

673

</page>

674

675

676

677

678

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

679

[f] [[Main Page]][/f]

680

681

682

!Basic detecting unit of the SEVAN network at NorAmberd

683

684

Page Under Construction.

685

686

687

688

689

{| border="1px"

690

[url="setups/asec/pictures/566px-SEVAN.jpg"][img]setups/asec/pictures/300px-SEVAN.jpg[/img][/url]

691

692

[i][b]Figure 1:[/b] The basic detecting unit of the SEVAN network.[/i]

693

694

695

696

697

698

699

!!Structure of the information content from SEVAN detector

700

701

The following information is providing by SEVAN detector:

702

703

*Count rates from the all 3 layers (see Table 16).

704

*Count rates of the all coincidences of upper, middle and lower detectors (see Table 16 and Table 17).

705

*Correlation matrix between all detected signals (Table 18)

706

707

In the directory “DEFAULT” the following information is stored:

708

709

*columns 1-3 - the count rates of all channels of the SEVAN. The count rates are posted in the Table 16;

710

*column 4 unused (this channel we can use as input of the atmospheric pressure sensor).

711

712

713

714

715

716

717

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

718

[f] [[Main Page]][/f]

719

</page>

720

721

722

723

724

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

725

[f] [[Main Page]][/f]

1025

1026

1027

1028

1029

[f] [b][[Main Page|Return to Main Page]][/b][/f]

1030

</page>

1031

1032

1033

1034

1035

[f] [b][[Main Page|Return to Main Page]][/b][/f]

726

1036

727

1037

728

1038

!Magnetometer.

729

1039

730

Page Unter Construction.

731

732

733

{| border="1px"

734

[url="setups/asec/pictures/LEMI-417.jpg"][img]setups/asec/pictures/LEMI-417.jpg[/img][/url]

735

736

[i][b]Figure 1:[/b] Magnetotelluric Station (MTS) Lemi-417.[/i]

737

738

739

Text

740

741

742

743

744

745

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

746

[f] [[Main Page]][/f]

747

</page>

748

749

750

751

752

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

753

[f] [[Main Page]][/f]

754

755

756

!Electric Field Monitor Boltek EFM100 NorAmberd

757

758

759

Page Under Construction.

760

761

762

{| border="1px"

763

[url="setups/asec/pictures/800px-BoltekEFM-100_Yerevan.JPG"][img]setups/asec/pictures/300px-BoltekEFM-100_Yerevan.JPG[/img][/url]

764

765

[i][b]Figure 1:[/b] Electric Field Monitor Boltek EFM100.[/i]

766

767

768

Text

769

770

771

772

773

774

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

775

[f] [[Main Page]][/f]

776

</page>

777

778

779

780

781

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

782

[f] [[Main Page]][/f]

783

784

785

!Lightning Detector Boltek LD NorAmberd

786

787

788

Page Under Construction.

789

790

791

{| border="1px"

792

[url="setups/asec/pictures/Anthand-t.jpg"][img]setups/asec/pictures/100px-Anthand-t.jpg[/img][/url]

793

794

[i][b]Figure 1:[/b] Lightning Detector Boltek LD250.[/i]

795

796

797

Page Under Construction.

798

799

800

801

802

803

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

804

[f] [[Main Page]][/f]

805

</page>

806

807

808

809

810

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

811

[f] [[Main Page]][/f]

1040

This page is under construction; however, information about the LEMI-018 Magnetometer can be found at the [url="http://www.isr.lviv.ua/lemi018.htm"]manufacturer's website[/url]. [br]

1041

1042

1043

{| border="1px"

1044

[url="http://www.isr.lviv.ua/lemi018.htm"][img]http://www.isr.lviv.ua/images/lemi018.jpg[/img][/url]

1045

1046

[i][b]Figure 1:[/b] Magnetometer LEMI-018.[/i]

1047

1048

1049

Text

1050

1051

1052

1053

1054

1055

1056

[f] [b][[Main Page|Return to Main Page]][/b][/f]

1057

</page>

1058

1059

1060

1061

1062

[f] [b][[Main Page|Return to Main Page]][/b][/f]

812

1063

813

1064

814

1065

!About CRD headquarters at Yerevan

827

1078

headquarters at A.I. Alikhanyan National Science Laboratory, Yerevan.

828

1079

829

1080

830

831

832

833

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

834

[f] [[Main Page]][/f]

835

</page>

836

837

838

839

840

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

841

[f] [[Main Page]][/f]

842

843

844

!Electric Field Monitor Boltek EFM100 Yerevan

845

846

847

Page Under Cinstruction.

848

849

850

{| border="1px"

851

[url="setups/asec/pictures/800px-BoltekEFM-100_Yerevan.JPG"][img]setups/asec/pictures/300px-BoltekEFM-100_Yerevan.JPG[/img][/url]

852

853

[i][b]Figure 1:[/b] Electric Field Monitor Boltek EFM100.[/i]

854

855

856

857

858

859

860

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

861

[f] [[Main Page]][/f]

862

</page>

863

864

865

866

867

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

868

[f] [[Main Page]][/f]

869

870

871

!Lightning Detector Boltek LD Yerevan

872

873

874

Page Under Construction.

875

876

877

{| border="1px"

878

[url="setups/asec/pictures/Anthand-t.jpg"][img]setups/asec/pictures/100px-Anthand-t.jpg[/img][/url]

879

880

[i][b]Figure 1:[/b] Lightning Detector Boltek LD250.[/i]

881

882

883

884

885

886

887

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

888

[f] [[Main Page]][/f]

889

</page>

890

891

892

893

894

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

895

[f] [[Main Page]][/f]

896

897

898

!Basic detecting unit of the SEVAN network at Yerevan

899

900

Page Under Construction.

901

902

903

904

905

{| border="1px"

906

[url="setups/asec/pictures/566px-SEVAN.jpg"][img]setups/asec/pictures/300px-SEVAN.jpg[/img][/url]

907

908

[i][b]Figure 1:[/b] The basic detecting unit of the SEVAN network.[/i]

909

910

911

912

913

914

915

!!Structure of the information content from SEVAN detector

916

917

The following information is providing by SEVAN detector:

918

919

*Count rates from the all 3 layers (see Table 16).

920

*Count rates of the all coincidences of upper, middle and lower detectors (see Table 16 and Table 17).

921

*Correlation matrix between all detected signals (Table 18)

922

923

In the directory “DEFAULT” the following information is stored:

924

925

*columns 1-3 - the count rates of all channels of the SEVAN. The count rates are posted in the Table 16;

926

*column 4 unused (this channel we can use as input of the atmospheric pressure sensor).

927

928

929

930

931

932

933

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

934

[f] [[Main Page]][/f]

935

</page>

936

937

938

939

940

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

941

[f] [[Main Page]][/f]

942

943

944

!Basic detecting unit of the SEVAN network at Burakan

945

946

Page Under Construction.

947

948

949

950

951

{| border="1px"

952

[url="setups/asec/pictures/566px-SEVAN.jpg"][img]setups/asec/pictures/300px-SEVAN.jpg[/img][/url]

953

954

[i][b]Figure 1:[/b] The basic detecting unit of the SEVAN network.[/i]

955

956

957

958

959

960

961

!!Structure of the information content from SEVAN detector

962

963

The following information is providing by SEVAN detector:

964

965

*Count rates from the all 3 layers (see Table 16).

966

*Count rates of the all coincidences of upper, middle and lower detectors (see Table 16 and Table 17).

967

*Correlation matrix between all detected signals (Table 18)

968

969

In the directory “DEFAULT” the following information is stored:

970

971

*columns 1-3 - the count rates of all channels of the SEVAN. The count rates are posted in the Table 16;

972

*column 4 unused (this channel we can use as input of the atmospheric pressure sensor).

973

974

975

976

977

978

979

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

980

[f] [[Main Page]][/f]

981

</page>

982

983

984

985

986

987

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

988

[f] [[Main Page]][/f]

989

990

991

!Basic detecting unit of the SEVAN network at Moussala

992

993

Page Under Construction.

994

995

996

997

998

{| border="1px"

999

[url="setups/asec/pictures/566px-SEVAN.jpg"][img]setups/asec/pictures/300px-SEVAN.jpg[/img][/url]

1000

1001

[i][b]Figure 1:[/b] The basic detecting unit of the SEVAN network.[/i]

1002

1003

1004

1005

1006

1007

1008

!!Structure of the information content from SEVAN detector

1009

1010

The following information is providing by SEVAN detector:

1011

1012

*Count rates from the all 3 layers (see Table 16).

1013

*Count rates of the all coincidences of upper, middle and lower detectors (see Table 16 and Table 17).

1014

*Correlation matrix between all detected signals (Table 18)

1015

1016

In the directory “DEFAULT” the following information is stored:

1017

1018

*columns 1-3 - the count rates of all channels of the SEVAN. The count rates are posted in the Table 16;

1019

*column 4 unused (this channel we can use as input of the atmospheric pressure sensor).

1020

1021

1022

1023

1024

1025

1026

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

1027

[f] [[Main Page]][/f]

1028

</page>

1029

1030

1031

1032

1033

1034

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

1035

[f] [[Main Page]][/f]

1036

1037

1038

!Basic detecting unit of the SEVAN network at Moussala

1039

1040

Page Under Construction.

1041

1042

1043

1044

1045

{| border="1px"

1046

[url="setups/asec/pictures/566px-SEVAN.jpg"][img]setups/asec/pictures/300px-SEVAN.jpg[/img][/url]

1047

1048

[i][b]Figure 1:[/b] The basic detecting unit of the SEVAN network.[/i]

1049

1050

1051

1052

1053

1054

1055

!!Structure of the information content from SEVAN detector

1056

1057

The following information is providing by SEVAN detector:

1058

1059

*Count rates from the all 3 layers (see Table 16).

1060

*Count rates of the all coincidences of upper, middle and lower detectors (see Table 16 and Table 17).

1061

*Correlation matrix between all detected signals (Table 18)

1062

1063

In the directory “DEFAULT” the following information is stored:

1064

1065

*columns 1-3 - the count rates of all channels of the SEVAN. The count rates are posted in the Table 16;

1066

*column 4 unused (this channel we can use as input of the atmospheric pressure sensor).

1067

1068

1069

1070

1071

1072

1073

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

1074

[f] [[Main Page]][/f]

1075

</page>

1076

1077

1078

1079

1080

1081

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

1082

[f] [[Main Page]][/f]

1083

1084

1085

!Basic detecting unit of the SEVAN network at Zagreb

1086

1087

Page Under Construction.

1088

1089

1090

1091

1092

{| border="1px"

1093

[url="setups/asec/pictures/566px-SEVAN.jpg"][img]setups/asec/pictures/300px-SEVAN.jpg[/img][/url]

1094

1095

[i][b]Figure 1:[/b] The basic detecting unit of the SEVAN network.[/i]

1096

1097

1098

1099

1100

1101

1102

!!Structure of the information content from SEVAN detector

1103

1104

The following information is providing by SEVAN detector:

1105

1106

*Count rates from the all 3 layers (see Table 16).

1107

*Count rates of the all coincidences of upper, middle and lower detectors (see Table 16 and Table 17).

1108

*Correlation matrix between all detected signals (Table 18)

1109

1110

In the directory “DEFAULT” the following information is stored:

1111

1112

*columns 1-3 - the count rates of all channels of the SEVAN. The count rates are posted in the Table 16;

1113

*column 4 unused (this channel we can use as input of the atmospheric pressure sensor).

1114

1115

1116

1117

1118

1119

1120

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

1121

[f] [[Main Page]][/f]

1122

</page>

1123

1124

1125

1126

1127

1128

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

1129

[f] [[Main Page]][/f]

1130

1131

1132

!Basic detecting unit of the SEVAN network at JNU

1133

1134

Page Under Construction.

1135

1136

1137

1138

1139

{| border="1px"

1140

[url="setups/asec/pictures/566px-SEVAN.jpg"][img]setups/asec/pictures/300px-SEVAN.jpg[/img][/url]

1141

1142

[i][b]Figure 1:[/b] The basic detecting unit of the SEVAN network.[/i]

1143

1144

1145

1146

1147

1148

1149

!!Structure of the information content from SEVAN detector

1150

1151

The following information is providing by SEVAN detector:

1152

1153

*Count rates from the all 3 layers (see Table 16).

1154

*Count rates of the all coincidences of upper, middle and lower detectors (see Table 16 and Table 17).

1155

*Correlation matrix between all detected signals (Table 18)

1156

1157

In the directory “DEFAULT” the following information is stored:

1158

1159

*columns 1-3 - the count rates of all channels of the SEVAN. The count rates are posted in the Table 16;

1160

*column 4 unused (this channel we can use as input of the atmospheric pressure sensor).

1161

1162

1163

1164

1165

1166

1167

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

1168

[f] [[Main Page]][/f]

1169

</page>

1170

1171

1172

1173

1174

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

1175

[f] [[Main Page]][/f]

1081

1082

1083

1084

1085

[f] [b][[Main Page|Return to Main Page]][/b][/f]

1086

</page>

1087

1088

1089

1090

1091

[f] [b][[Main Page|Return to Main Page]][/b][/f]

1176

1092

1177

1093

1178

1094

!Cube_3cm

1186

1102

Page Under Construction

1187

1103

1188

1104

1189

1190

1191

1192

[f] [[SEVAN Monitors]] | [[SEVAN Moussala]] | [[SEVAN Zagreb]] | [[SEVAN JNU]] [/f] [br]

1193

[f] [[Main Page]][/f]

1105

1106

1107

1108

1109

[f] [b][[Main Page|Return to Main Page]][/b][/f]

1194

1110

</page>

1195

1196

1197

1111

1198

1112

!UI Usage Guide | [[Main Page]]

1199

1113

ADEI provides sophisticated Google-maps style web interface. The short video displaying basic functionality could be obtained from [url="http://csa.aragats.am/ADEI.mpeg"] here[/url].

1200

1114

!!Selecting Data

1222

1136

* Moving

1223

1137

* Swipe Left - Moves a step forward in time-axis (x-axis).

1224

1138

* Swipe Right - Moves a step backward in time-axis(x-axis).

1225

* Swip Up - Moves a step down in y-axis.

1139

* Swipe Up - Moves a step down in y-axis.

1226

1140

* Swipe Down - Moves a step up in y-axis.

1227

1141

!!Legend

1228

1142

The graph is containing information on displayed [i]LogGroup[/i], time range, aggregating parameters, but the actual channel names are not shown in order to save space. The Legend window is used to provide information on the items. Clicking with left mouse button at the graph window will open popup window listing the names of all data channels whose plots passing near to the clicked point.

1248

1162

1249

1163

[[Main Page]]

1250

1164

</page>

1251

1252

1165

1166

1167

1168

1169

1170

1171

1172

[f] [b][[Main Page|Return to Main Page]][/b][/f]

1173

1174

{| border="1px"

1175

[br]

1176

[br][u][b]"2009-09-19"[/b][/u] [b]ASNT, 5cm detetors 5,6,7,8[/b]

1177

[br][preview(db_server=ar&amp;db_name=raw&amp;db_group=ASNT_AR&amp;db_mask=4,5,6,7&amp;window=1253397600-1253402159&amp;width=400&amp;height=120), link]

1178

[br]

1179

[br][u][b]"2010-10-04"[/b][/u] [b]ASNT, 5cm detetors 5,6,7,8[/b]

1180

[br][preview(db_server=ar&amp;db_name=raw&amp;db_group=ASNT_AR&amp;db_mask=4,5,6,7&amp;window=1286215800-1286217000&amp;width=400&amp;height=120), link]

1181

[br]

1182

[br][u][b]"2011-04-20"[/b][/u] [b]Stand_1cm, Coincidence 100[/b]

1183

[br][preview(db_server=ar&amp;db_name=raw&amp;db_group=Stand_1cm_AR&amp;db_mask=8&amp;window=1303277400-1303300800&amp;width=400&amp;height=120), link]

1184

[br]

1185

[br][u][b]"2011-05-07"[/b][/u] [b]ASNT, 60cm detetor 1[/b]

1186

[br][preview(db_server=ar&amp;db_name=raw&amp;db_group=ASNT_AR&amp;db_mask=0&amp;window=1304775900-1304777400&amp;width=400&amp;height=120), link]

1187

[br]

1188

[br][u][b]"2011-06-04"[/b][/u] [b]Stand_1cm, detector 1[/b]

1189

[br][preview(db_server=ar&amp;db_name=raw&amp;db_group=Stand_1cm_AR&amp;db_mask=0&amp;window=1307147400-1307154600&amp;width=400&amp;height=120), link]

1190

[br]

1191

[br][u][b]"2011-07-19"[/b][/u]

1192

[br]

1193

[br][u][b]"2011-08-21"[/b][/u]

1194

[br]

1195

[br][u][b]"2012-06-12"[/b][/u]

1196

[br]

1197

[br][u][b]"2012-09-14"[/b][/u]

1198

[br]

1199

[br][u][b]"2012-10-07"[/b][/u]

1200

[br]

1201

[br][u][b]"2012-10-18"[/b][/u]

1202

[br]

1203

[br][u][b]"2013-01-08"[/b][/u]

1204

[br]

1205

[br][u][b]"2013-09-19"[/b][/u]

1206

[br]

1207

[br][u][b]"2013-10-19"[/b][/u]

1208

[br]

1209

[br][u][b]"2014-04-16"[/b][/u]

1210

[br]

1211

[br][u][b]"2014-04-25"[/b][/u]

1212

[br]

1213

[br][u][b]"2014-04-27"[/b][/u]

1214

[br]

1215

[br][u][b]"2014-04-28"[/b][/u] [b]Stand_1cm, detector 1[/b]

1216

[br][preview(db_server=ar&amp;db_name=raw&amp;db_group=Stand_1cm_AR&amp;db_mask=0&amp;window=1398691800-1398699900&amp;width=400&amp;height=120), link]

1217

[br]

1218

[br][u][b]"2014-05-26"[/b][/u] [b]Stand_1cm, detector 1[/b]

1219

[br][preview(db_server=ar&amp;db_name=raw&amp;db_group=Stand_1cm_AR&amp;db_mask=0&amp;window=1401094800-1401138000&amp;width=400&amp;height=120), link]

1220

[br]

1221

[br][u][b]"2014-06-02"[/b][/u] [b]Stand_1cm, detector 1[/b]

1222

[br][preview(db_server=ar&amp;db_name=raw&amp;db_group=Stand_1cm_AR&amp;db_mask=0&amp;window=1401703200-1401771600&amp;width=400&amp;height=120), link]

1223

[br]

1224

[br][u][b]"2014-10-04"[/b][/u] [b]ASNT, 5cm detetors 5,6,7,8[/b]

1225

[br][preview(db_server=ar&amp;db_name=raw&amp;db_group=ASNT_AR&amp;db_mask=4,5,6,7&amp;window=1412430900-1412432700&amp;width=400&amp;height=120), link]

1226

[br]

1227

[br][u][b]"2015-03-30"[/b][/u] [b]Stand_1cm, detector 1[/b]

1228

[br][preview(db_server=ar&amp;db_name=raw&amp;db_group=Stand_1cm_AR&amp;db_mask=0&amp;window=1427712600-1427718300&amp;width=400&amp;height=120), link]

1229

1230

[br]

1231

[br][u][b]"2015-04-04"[/b][/u]

1232

[br]

1233

[br][u][b]"2015-04-09"[/b][/u]

1234

[br]

1235

[br][u][b]"2015-04-19"[/b][/u]

1236

[br]

1237

[br][u][b]"2015-04-20"[/b][/u]

1238

[br]

1239

[br][u][b]"2015-04-21"[/b][/u]

1240

[br]

1241

[br][u][b]"2015-04-23"[/b][/u]

1242

[br]

1243

[br][u][b]"2015-04-28"[/b][/u]

1244

[br]

1245

[br][u][b]"2015-05-10"[/b][/u]

1246

[br]

1247

[br][u][b]"2015-05-11"[/b][/u]

1248

[br]

1249

[br][u][b]"2015-05-13"[/b][/u]

1250

[br]

1251

[br][u][b]"2015-05-23"[/b][/u]

1252

[br]

1253

[br][u][b]"2015-05-25"[/b][/u]

1254

[br]

1255

[br][u][b]"2015-05-28"[/b][/u]

1256

[br]

1257

[br][u][b]"2015-06-03"[/b][/u]

1258

[br]

1259

[br][u][b]"2015-06-06"[/b][/u]

1260

[br]

1261

[br][u][b]"2015-06-09"[/b][/u]

1262

[br]

1263

[br][u][b]"2015-06-15"[/b][/u]

1264

[br]

1265

[br][u][b]"2015-06-18"[/b][/u]

1266

[br]

1267

[br][u][b]"2015-06-24"[/b][/u]

1268

[br]

1269

[br][u][b]"2015-06-25"[/b][/u]

1270

[br]

1271

[br][u][b]"2015-07-06"[/b][/u]

1272

[br]

1273

[br][u][b]"2015-07-17"[/b][/u]

1274

[br]

1275

[br][u][b]"2015-07-24"[/b][/u]

1276

[br]

1277

[br][u][b]"2015-08-02"[/b][/u]

1278

[br]

1279

[br][u][b]"2015-08-03"[/b][/u]

1280

[br]

1281

[br][u][b]"2015-08-06"[/b][/u]

1282

[br]

1283

[br][u][b]"2015-08-07"[/b][/u]

1284

[br]

1285

[br][u][b]"2015-08-08"[/b][/u]

1286

[br]

1287

[br][u][b]"2015-08-22"[/b][/u]

1288

[br]

1289

[br][u][b]"2015-08-23"[/b][/u]

1290

[br]

1291

[br][u][b]"2015-08-24"[/b][/u]

1292

[br]

1293

[br][u][b]"2015-08-25"[/b][/u]

1294

[br]

1295

[br][u][b]"2015-08-26"[/b][/u]

1296

[br]

1297

[br][u][b]"2015-08-28"[/b][/u]

1298

[br]

1299

[br][u][b]"2015-08-31"[/b][/u]

1300

[br]

1301

[br][u][b]"2015-10-07"[/b][/u]

1302

[br]

1303

[br][u][b]"2015-11-11"[/b][/u]

1304

[br]

1305

[br][u][b]"2015-11-12"[/b][/u]

1306

[br]

1307

[br][u][b]"2015-11-13"[/b][/u]

1308

[br]

1309

[br][u][b]"2015-11-14"[/b][/u]

1310

1311

[br]

1312

[br][u][b]"2016-03-04"[/b][/u] [b]Boltek EFM100, MAKET[/b]

1313

[br][preview(db_server=ar&amp;db_name=raw&amp;db_group=Electric_Field_MAKET_AR&amp;db_mask=0&amp;window=1457116500-1457120100&amp;width=400&amp;height=120), link]

1314

[br]

1315

[br][u][b]"2016-04-28"[/b][/u] [b]Boltek EFM100, MAKET[/b]

1316

[br][preview(db_server=ar&amp;db_name=raw&amp;db_group=Electric_Field_MAKET_AR&amp;db_mask=0&amp;window=1461866100-1461869700&amp;width=400&amp;height=120), link]

1317

[br]

1318

[br][u][b]"2016-05-04"[/b][/u] [b]Boltek EFM100, MAKET[/b]

1319

[br][preview(db_server=ar&amp;db_name=raw&amp;db_group=Electric_Field_MAKET_AR&amp;db_mask=0&amp;window=1462386900-1462390500&amp;width=400&amp;height=120), link]

1320

[br]

1321

[br][u][b]"2016-05-12"[/b][/u] [b]Boltek EFM100, MAKET[/b]

1322

[br][preview(db_server=ar&amp;db_name=raw&amp;db_group=Electric_Field_MAKET_AR&amp;db_mask=0&amp;window=1463059800-1463063400&amp;width=400&amp;height=120), link]

1323

[br]

1324

[br][u][b]"2016-05-15"[/b][/u] [b]Boltek EFM100, MAKET[/b]

1325

[br][preview(db_server=ar&amp;db_name=raw&amp;db_group=Electric_Field_MAKET_AR&amp;db_mask=0&amp;window=1463278200-1463281800&amp;width=400&amp;height=120), link]

1326

[br]

1327

[br][u][b]"2016-06-04"[/b][/u] [b]Boltek EFM100, MAKET[/b]

1328

[br][preview(db_server=ar&amp;db_name=raw&amp;db_group=Electric_Field_MAKET_AR&amp;db_mask=0&amp;window=1465002000-1465005600&amp;width=400&amp;height=120), link]

1329

[br]

1330

[br][u][b]"2016-06-08"[/b][/u] [b]Boltek EFM100, GAMMA[/b]

1331

[br][preview(db_server=ar&amp;db_name=raw&amp;db_group=Electric_Field_Monk_AR&amp;db_mask=0&amp;window=1465384200-1465387800&amp;width=400&amp;height=120), link]

1332

[br]

1333

[br][u][b]"2016-06-11"[/b][/u] [b]Boltek EFM100, MAKET[/b]

1334

[br][preview(db_server=ar&amp;db_name=raw&amp;db_group=Electric_Field_MAKET_AR&amp;db_mask=0&amp;window=1465643400-1465647000&amp;width=400&amp;height=120), link]

1335

[br]

1336

[br][u][b]"2016-06-16"[/b][/u] [b]Boltek EFM100, MAKET[/b]

1337

[br][preview(db_server=ar&amp;db_name=raw&amp;db_group=Electric_Field_MAKET_AR&amp;db_mask=0&amp;window=1466069400-1466073000&amp;width=400&amp;height=120), link]

1338

[br]

1339

[br][u][b]"2016-07-28"[/b][/u] [b]Boltek EFM100, MAKET[/b]

1340

[br][preview(db_server=ar&amp;db_name=raw&amp;db_group=Electric_Field_MAKET_AR&amp;db_mask=0&amp;window=1469712600-1469716200&amp;width=400&amp;height=120), link]

1341

[br]

1342

1343

1344

[[Main Page]]

1345

</page>

1346

1347

1348

1349

1350

1351

1253

1352

</pages>

1254

1353

<<>>-->

b'\\ No newline at end of file'

Older »