Geophysical Research Network operating in the Aragats Space Environmental Center A. Chilingaryan 1, K. Arakelyan 1, S. Chilingarian 2, A. Reymers 1 1 A.

Slides:



Advertisements
Similar presentations
Anisotropy in Cosmic Ray Arrival Directions Using IceCube and IceTop Frank McNally ISCRA.
Advertisements

Antonis Leisos KM3NeT Collaboration Meeting the calibration principle using atmospheric showers the calibration principle using atmospheric showers Monte.
Investigation of daily variations of cosmic ray fluxes in the beginning of 24 th solar activity cycle Ashot Chilingarian, Bagrat Mailyan IHY-ISWI Regional.
Cosmic Ray Using for Monitoring and Forecasting Dangerous Solar Flare Events Lev I. Dorman (1, 2) 1. Israel Cosmic Ray & Space Weather Center and Emilio.
Hybrid Extensive Air Shower Detector Array at the University of Puebla to Study Cosmic Rays O. MARTINEZ, H. SALAZAR, L. VILLASEÑOR * + Grupo de Estudiantes.
Use of floating surface detector stations for the calibration of a deep-sea neutrino telescope G. Bourlis, N. A. B. Gizani, A. Leisos, A. G. Tsirigotis,
Cosmic Rays Basic particle discovery. Cosmic Rays at Earth – Primaries (protons, nuclei) – Secondaries (pions) – Decay products (muons, photons, electrons)
A.Chilingarian Particle detectors networks for the Fundamental Physics, Space Weather and Education Cosmic Ray Division, Alikhanyan Physics Institute,Yerevan,
Terrestrial gamma-ray flashes Prepared by Morris Cohen Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global AWESOME Network.
Multiple lasers strike the fusion Target. A variety of particles are ultimately released (including tertiary neutrons). Carbon sensor is activated by neutrons;
H.E.G.R.A. High Energy Gamma Ray Astronomy By: Lisa Busing.
1 Gamma-Ray Astronomy with GLAST May 24, 2008 Toby Burnett WALTA meeting.
Cosmic Ray Workshop May 15, May 15, 2010 Rutgers Cosmic Ray Workshop.
Athens 27 September 2007 The S.V.I.R.CO. Observatory (INAF/UNIROMA3 Collaboration): Present status Workshop on Neutron Monitors 'The present and the future.
Detection of MeV electrons, neutrons and gammas from the Relativistic Feedback Breakdown Process by particle detectors at Aragats A.Chilingarian.
COST ES0803 WG2 report. National contributions to activities Received reports from T. Breus, D. Heynderickx, A. Chilingarian, N. Jakowski, H. Haralambous,
Update on Corsika Simulation 29 June 2015 Fabrizio Coccetti 1.
RELEC project (Relativistic ELECtrons). Unified platform “Karat” for small spacecraft 2 MICROSATELLITE KARAT FOR PLANETARY MISSIONS, ASTROPHYSICAL AND.
Status of Cosmic Rays Physics at the Knee Andrea Chiavassa Università and INFN Torino NOW 2006 Otranto 9-16 September 2006.
1 Alessandra Casale Università degli Studi di Genova INFN Sezione Genova FT-Cal Prototype Simulations.
QuarkNet Muon Data Analysis with Shower Array Studies J.L. FISCHER, A. CITATI, M. HOHLMANN Physics and Space Sciences Department, Florida Institute of.
Lightning Detection at Aragats Station
Size and Energy Spectra of incident cosmic radiation obtained by the MAKET - ANI surface array on mountain Aragats. (Final results from MAKET-ANI detector)‏
● The Roland Maze Project: School-Based Extensive Air Shower Network ● Hands on CERN events J. Szabelski The Andrzej Soltan Institute for Nuclear Studies,
222Rn daughters influence on scaler mode of ARGO-YBJ detector Irene Bolognino, University of Pavia and INFN E. Giroletti,C. Cattaneo,G. Liguori,P. Salvini,P.
Preliminary MC study on the GRAND prototype scintillator array Feng Zhaoyang Institute of High Energy Physics, CAS, China GRAND Workshop, Paris, Feb. 015.
Events 1. Figure 4 shows: Left panel – Negative values ​​ of the electric field and data of high energy neutrons (upper panel), thermal neutrons (lower.
The short particle bursts during thunderstorms: EAS or lightning seeds? G. Hovsepyan, A. Chilingarian, A. Alikhanian National Laboratory, Armenia.
1 IGY The ALERT signal of ground level enhancements of solar cosmic rays: physics basis, the ways of realization and development Anashin V., Belov A.,
Teaching and Learning with the Cosmic Ray e-Lab
Spectra of the Thunderstorm Correlated Electron and Gamma-Ray Measured at Aragats Bagrat Mailyan and Ashot Chilingarian.
Operation of the Space Environmental viewing and Analysis Network (Sevan) in 24-th Solar Activity Cycle A. Chilingarian A. Chilingarian Yerevan Physics.
Gus Sinnis Asilomar Meeting 11/16/2003 The Next Generation All-Sky VHE Gamma-Ray Telescope.
Exploitation of Space Ionizing Radiation Monitoring System in Russian Federal Space Agency STRUCTURE OF THE MONITORING SYSTEM The Monitoring System includes.
Multi-TeV  -ray Astronomy with GRAPES-3 Pravata K Mohanty On behalf of the GRAPE-3 collaboration Tata Institute of Fundamental Research, Mumbai Workshop.
Aa GLAST Particle Astrophysics Collaboration Instrument Managed and Integrated at SLAC/Stanford University The Gamma-ray Large Area Space Telescope (GLAST)
Cosmic rays at sea level. There is in nearby interstellar space a flux of particles—mostly protons and atomic nuclei— travelling at almost the speed of.
The Andrzej Soltan Institute for Nuclear Studies, Cosmic Ray Laboratory, ul. Uniwersytecka 5, Lodz, P.O.Box 447, Poland Pylos,
Variations of Cosmic Rays during Thunderstorms N.S. Khaerdinov & A. S. Lidvansky Institute for Nuclear Research, Russian Academy of Sciences, Moscow, Russia.
On the origin of the huge natural electron accelerators operated in the thunderclouds Ashot Chilingarian Artem Alikhanyan National Laboratory (Yerevan.
2015 ASEC Data Electric field and lightning occurrences: now at Aragats 3 EFM-100 and 2 NextStorms – comparisons analysis – physical inference; LONG and.
A Future All-Sky High Duty Cycle VHE Gamma Ray Detector Gus Sinnis/Los Alamos with A. Smith/UMd J. McEnery/GSFC.
Median Filtering Algorithms for Multichannel Detectors and their influence on Thunderstorm Peaks in Cosmic Ray Data Armen Hovhannisyan Alikhanyan Physics.
Space Environmental Viewing and Analysis Network (SEVAN) Chilingarian 1, Ch.Angelov 2, K. Arakelyan 1, T.Arsov 2, Avakyan 1, S. Chilingaryan 1,4, K. A.Hovhanissyan.
High-energy Electron Spectrum From PPB-BETS Experiment In Antarctica Kenji Yoshida 1, Shoji Torii 2 on behalf of the PPB-BETS collaboration 1 Shibaura.
Physical Description of IceTop 3 Nov IceTop Internal Review Madison, November 3-4, 2010 Physical Description of IceTop Paul Evenson, University.
Some results of observation of ultraviolet and infrared emission from lightning discharges at Aragats Cosmic Station LEAD workshop Armenia, NOR AMBERD.
The KASCADE-Grande Experiment: an Overview Andrea Chiavassa Universita’ di Torino for the KASCADE-Grande Collaboration.
The Gulmarg Neutron Monitor Ramesh Koul Astrophysical Sciences Division Bhabha Atomic Research Centre Mumbai
Registration of the KeV and MeV neutron burst associated with thunderstorms or lightning Ashot Chilingaryan and Nikolay Bostanjyan A. Alikhanyan National.
Performances of the KM2A prototype array J.Liu for the LHAASO Collaboration Institute of High Energy Physics, CAS 32nd International Cosmic Ray Conference,
Gamma-ray Large Area Space Telescope -France -Germany -Italy -Japan -Sweden -USA Energy Range 10 keV-300 GeV. GLAST : - An imaging gamma-ray telescope.
Lingling Ma IHEP China Measurement of Cosmic rays with LHAASO at 10PeV~100PeV 4th Workshop on Air Shower Detection at High Altitude Institute of High Energy.
April 4 TGE – mostly electrons! Ne/Ngamma ~ 2!!!! 3 hours long TGE at low energies STAND1 MAKET – under deep snow! EFM 100 GAMMA – very large disturbances.
Periodic Variations in Muon Flux at Project GRAND Thomas A. Catanach, John Poirier ICRC August 2011.
1 Cosmic Ray Physics with IceTop and IceCube Serap Tilav University of Delaware for The IceCube Collaboration ISVHECRI2010 June 28 - July 2, 2010 Fermilab.
CHANDLER Detector Neutronics Modeling Alireza Haghighat William Walters Nuclear Science and Engineering Lab (NSEL) Nuclear Engineering Program, Mechanical.
Neutron emission in TGE’s L.Vanyan*, A.Chilingaryan, N.Bostanjyan, T.Karapetyan Yerevan Physics Institute.
Happy 2016!. Inverse polarity electric field at Aragats!
Modeling of secondary cosmic ray spectra for Solar Cycles 23
The “Carpet-2” multipurpose air shower array of the Baksan Neutrino Observatory INR of RAS A.U. Kudzhaev Institute for Nuclear Research, Russian Academy.
an open source detector for cosmic rays
A.S. Lidvansky, M.N. Khaerdinov, N.S. Khaerdinov
THEMIS and Space Weather
Department of Space Physics: Detached Laboratory at Lomnický štít (LS)
an open source detector for cosmic rays
on behalf of the GAMMA Collaboration
Higgs Factory Backgrounds
Estimation of Sensitivity to Gamma Ray point Sources above 30TeV
Bagrat Mailyan, Alikhanian National Laboratory (Former YerPhI)
Presentation transcript:

Geophysical Research Network operating in the Aragats Space Environmental Center A. Chilingaryan 1, K. Arakelyan 1, S. Chilingarian 2, A. Reymers 1 1 A. Alikhanian National Laboratory, Armenia 2 A. Alikhanian National Laboratory and Karlsruhe Institute of Technology, Germany

Aragats Station Altitude 3200m above sea level. Geographical coordinates is 40 o 28'N, 44 o 10'E, RC=7.1GV

15 Monitors at Aragats AMMM SEVAN Cube Stand_3cm Stand Electric Field Weather Station Lightning Detector Magnetic and Telluric Filed NaI(Tl) Geiger Antenna

Aragats high altitude research station Total number of monitors at station – 15 Number of physical channels – 200. Number of software channels – 581. Type of measurements – Cosmic ray fluxes, Geomagnetic field, Electrical field, Lightning types and distances, Weather parameters. Type of Detectors – Organic and inorganic scintillatiors (Plastic and NaI crystal), Geiger and Proportional counters, Fluxgate, Electrical field mills, Direction-finding antenna, other sensors. Measured parameters of the Cosmic ray fluxes: Electrons and muons with energy thresholds – 2,4,7,9,12,15,18,25,35,100 MeV. High energy muons with energy > 5GeV; > 250MeV. Gamma Rays. Thermal and MeV neutrons. Extensive Air shower corresponding to primary energies TeV. Horizontal muons within acceptance of 0 +/- 0.5 degree. Histograms of energy deposits. Event selection according to chosen triggering conditions; possibility to change scale of time series from 1 second to 1 minute.

Nor-Amberd Station Altitude 2000m above sea level. Geographical coordinates is 40 o 22'N, 44 o 15'E, RC=7.1GV

SEVAN 9 Monitors at Nor-Amberd Magnetic Filed Electric Field Weather Station Lightning Detector Geiger

Monitors located at Nor-Amberd station Total number of monitors at station – 9. Number of physical channels – 59. Number of software channels – 384. Type of measurements – Cosmic ray fluxes, Geomagnetic field, Electrical field, Lightning types and distances, Weather parameters. Type of Detectors – Scintillatiors, Proportional and Geiger counters, Fluxgate, Electrical field mill, Direction-finding antenna, other sensors. Measured parameters of Cosmic ray fluxes: Electrons and muons with energy threshold – 10, 15 MeV. Muons with energy > 350MeV; 12 angular bins of the arriving muons Gamma rays. Thermal and MeV neutrons. 1-minute histograms of energy deposits. Flexible system of different event selection according to chosen triggering conditions; possibility to change scale of time series from 1 second to 1 minute

Yerevan headquarters Altitude 1000m above sea level. Geographical coordinates is 40 o 22'N, 44 o 15'E, RC=7.1GV

SEVAN Cube_3cm Monitors at Yerevan headquarters Electric Field Lightning Detector Total number of monitors at station – 4. Number of physical channels – 14. Number of software channels – 79. Type of measurements – Cosmic ray fluxes, Electrical field, Lightning types and distances, Weather parameters Type of Detectors – Plastic scintillatiors, NaI crystal, Electrical field mill, Direction-finding antenna, other sensors. Measured parameters of Cosmic ray fluxes: Electrons and muons with energy threshold – 7, 15, 20 MeV MeV. Muons with energy > 250MeV Neutrons and Gamma rays. Other Features: 1-minute histograms of energy deposits. Flexible system of different event selection according to chosen triggering conditions; possibility to change scale of time series from 1 second to 1 minute

Bulgaria, Mt. Musala, 42°10'45"N, 23°35'8"E, 2925m asl Croatia, Zagreb, 45°49'7"N, 15°58'30"E 160m asl India, Jawaharlal Nehru University, 28°32'26"N, 077°09'46"E, 258m asl SEVAN Monitors abroad

At this moment, geophysical research network consist from 31 monitors, 342 physical channels and 1063 software channels. Data size of ASEC GP network

Advanced Data Extraction Infrastructure (ADEI)