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Ashot Chilingarian
Survey Information
Institution: Yerevan Physics Institute
Organizational Affiliation:
Observations
Providing Observations for WHI: Yes
Observatory: Aragets Space Environmental Center (ASEC)
Type of Observation: particle monitors
Coverage for WHI: altitudes 1000, 2000 and 3200 m,
(4025N, 4415E; Vertical cut-off rigidity in 2007: 7.1 GV)
Observation Location for WHI:
Observation Plans for WHI: Flux of secondary cosmic rays measured by particle detectors, reflects the
"primary" cosmic ray flux incident on terrestrial atmosphere, which in
turn is directly connected with dynamics of the heliosphere.
Cosmic ray fluxes measured at minimal Solar Activity will comprise a
benchmark for further physical analysis of solar modulation events (Ground
Level Enhancements, Geomagnetic storms, Forbush decreases) expected during
24th solar cycle).
Particle monitors located at Aragats Space Environmental Center (ASEC) at
altitudes 1000, 2000 and 3200 m,
(4025N, 4415E; Vertical cut-off rigidity in 2007: 7.1 GV)
detect charged and neutral components of the secondary cosmic rays with
different energy thresholds and various angles of incidence. ASEC monitors
were equipped recently with new DAQ electronics and software significantly
enlarging its nformation content.
Sample Data File
Sample Image
Modeling
Providing Modeling Support for WHI: No
Model Name:
Model Web Site:
Type of Model:
Model Coverage:
Sample Model Output
Sample Model Image
Data
Assisting with Data Coordination: No
Data Service:
Data Service Website:
Service Type:
Data Types or Sources:
Organizational Affiliation:
Other
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