SW Publications

2011:

·         Calculation of the barometric coefficients at the start of the 24th solar activity cycle for particle detectors of Aragats Space Environmental Center

2010:

·         On the relation of the Forbush decreases detected by ASEC monitors during the 23rd solar activity cycle with ICME parameters

2009:

·         Cosmic ray intensity increases detected by Aragats Space Environmental Center monitors during the 23rd solar activity cycle in correlation with geomagnetic storms

·         Statistical study of the detection of solar protons of highest energies at 20 January 2005

 

2008:

·         Dudok de Wit, A. A. Chilingarian, Using neutron monitor network data to improve the detection of space weather events, COST  724 final report, pp.148-152, 2008.

·         G.G. Karapetyan, Detection of high energy solar protons during ground level enhancements, Astropart.Phys30 (2008) 234–238. (2008),

·         Y. Muraki, Y. Matsubara, S. Masuda et al. Detection of high-energy solar neutrons and protons by groundlevel detectors on April 15, 2001, Astroparticle Physics 29 (2008), pp. 229–242

2007:

·         A. Chilingarian, L. Melkumyan, G. Hovsepyan, A. Reymers, The response function of the Aragats Solar Neutron Telescope, Nuclear Instruments and Methods in Physics Research A 574 (2007) 255-263

·         Bostanjyan, N.K. et al., On the production of highest energy solar protons at 20 January 2005, J. Adv. Space Res. 39 (2007) 1456-1459.

·         A.A. Chilingarian, A.E. Reymers, Particle detectors in Solar Physics and Space Weather research, Astroparticle Physics (2007), Astropart. Phys., 27, pp 465-472

 

 2006:

·         Y. Muraki et al., Detection of Solar Neutrons and Protons by Ground Level Detectors, Proceedings of the 20th European Cosmic Ray Symposium in Lisbon, Portugal

2005:

·         A.Chilingarian for the ASEC team, (2005) Correlated Measurements of Secondary Cosmic Ray Fluxes by the Aragats Space- Environmental Center Monitors,NIM-A, 543, 483-496

·         N.Gevorgyan for the ASEC team, (2005) Test Alert Service Against Very Large SEP Events, Advances in Space Research (ASR), Vol. 36, issue 12, pp 2351-2356

·         A.Chilingarian, V. Babayan, V. Eganov, N. Bostanjyan, G. Karapetyan et al., (2005) The Mutual Treatment of 28-29.10.2003 Events by the ASEC Surface Monitors and Space-born Spectrometers on Board of ACE GOE Satellites, Proceedings of the Russian Academy of Science, Physics series, 69, 815-817.

·         H. S. Martirosyan (2005) Solar Flare Classification Attempt by SEP: I. Classification according to Knee Energies of SEP Ion Spectra, Astrophysica, 48, 247-260.

·         E. O. Flueckiger, R. Butikofer, A. Chilingarian, G. Hovsepyan, Y. H. Tan, (2005)Solar Neutron Events that Have Been Found in Solar Cycle 23, International Journal of Modern Physics A, Vol. 20, No.29., 6646-6650

 

2004:

·         H. Mavromichalaki, V. Yanke, L. Dorman, N. Iucci, A. Chilingaryan, O. Kryakunova, (2004)Neutron Monitor Network in Real Time and Space Weather, NATO Science Series monograph, "Effects of Space Weather on Technology Infrastructure",ed. by I.A. Daglis, Kluwer Academic Publishers, pp. 301-317

 

2003:

·         A.Chilingarian for the ASEC team, Monitoring and Forecasting of the Geomagnetic and Radiation Storms During the 23rd Solar Cycle. Aragats Regional Space Weather Center, Advances in Space Research, Vol. 31 (2003), pp 861-865.