Solar-terrestrial connections library
1. Solar flare of 15 February 2011 and its geomagnetic effects;
R.P. Kane, Instituto Nacional de
Pesquisas Espaciais (INPE)
2. Ionospheric effects of the solar flare of 15 February 2011;
R.P. Kane, Instituto Nacional de
Pesquisas Espaciais (INPE)
3. Ionospheric effects of the solar flare of 15 February 2011;
R.P. Kane, Instituto Nacional de
Pesquisas Espaciais (INPE)
4. Geomagnetic storm's precursors observed from 2001 to 2007 with
the Global Muon Detector Network (GMDN);
M. Rockenbach,1 A. Dal Lago2 W. D. Gonzalez,2 K. Munakata,3C. Kato, 3 T. Kuwabara, 4J.
Bieber, 4 N.
J. Schuch, 5 M.
L. Duldig, 6 J.
E. Humble, 6 H.
K. Al Jassar, 7 M. M. Sharma, 7 and I. Sabbah8,9
1 . Instituto de Pesquisa e Desenvolvimento, Universidade do
Vale do Paraíba, São José dos Campos, Brazil. 2. National Institute for Space
Research, São José dos Campos, Brazil. 3. Department of Physics, Shinshu
University, Matsumoto, Japan. 4. Bartol Research Institute and Department of
Physics and Astronomy, University of Delaware, Newark, Delaware, USA. 5. Southern
Regional Space Research Center, CRS/CCR/INPEMCT, Santa Maria, RS, Brazil. 6. School
of Mathematics and Physics, University of Tasmania, Hobart, Tasmania,
Australia. 7. Physics Department, Kuwait University, Kuwait. 8. Department of
Natural Sciences, College of Health Sciences, Public Authority of Applied
Education and Training, Kuwait City, Kuwait. 9. Department of Physics, Faculty
of Science, University of Alexandria, Alexandria, Egypt.
5. Migrating source of energetic radiation generated by thunderstorm activity;
Tatsuo Torii, 1 Takeshi Sugita, 1 Masashi
Kamogawa, 2 Yasuyuki Watanabe, 2 and Kenichi Kusunoki3
1 . Japan Atomic Energy Agency, Tokyo, Japan, 2. 2Department
of Physics, Tokyo Gakugei University, Tokyo, Japan, 3. Meteorological Research Institute, Tsukuba,
Japan.
6. Long‐duration gamma ray emissions from 2007 and 2008 winter
thunderstorms
H. Tsuchiya, 1 T. Enoto, 2 S. Yamada,3 T. Yuasa,
3 K. Nakazawa, 3 T. Kitaguchi, 4 M. Kawaharada, 5 M. Kokubun, 5 H. Kato, 1
M. Okano, 1 and K. Makishima
3
1 . High‐energy Astrophysics Laboratory, RIKEN, Wako, Japan;
2 . Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics
and SLAC National Accelerator Laboratory, Stanford University, Stanford,
California, USA; 3. Department of Physics, University of Tokyo, Tokyo, Japan; 4.
Division of Physics, Mathematics, and Astronomy, California Institute of Technology,
Pasadena, California, USA; 5. Department of High Energy Astrophysics, Institute
of Space and Astronautical Science, JAXA, Sagamihara, Japan.
7.
On the relation of the Forbush decreases detected by ASEC
monitors during the 23rd solar activity cycle with ICME parameters
A. Chilingarian, N. Bostanjyan; Cosmic Ray Division, Alikhanyan
National Laboratory, Yerevan, Armenia
8. Cosmic ray intensity increases detected by Aragats Space
Environmental Center monitors during the 23rd solar activity cycle in
correlation with geomagnetic storms
A. Chilingarian, N. Bostanjyan; Cosmic Ray Division, Alikhanyan
National Laboratory, Yerevan, Armenia
9. Investigation of diurnal variations of cosmic ray fluxes
measured with using ASEC and NMDB monitors
Bagrat Mailyan, Ashot Chilingarian; Cosmic Ray Division, Alikhanyan
National Laboratory, Yerevan,
Armenia
10. Calculations of the sensitivity of the particle detectors of
ASEC and SEVAN networks to galactic and solar cosmic rays
M. Zazyan, A.
Chilingarian; Cosmic Ray Division,
Alikhanyan National Laboratory, Yerevan, Armenia
11. Statistical study of the detection of solar protons of
highest energies at 20 January 2005
A. Chilingarian; Cosmic Ray Division, Alikhanyan
National Laboratory, Yerevan,
Armenia
12.
On the production of highest energy solar protons at 20
January 2005
N.Kh. Bostanjyan, A.A. Chilingarian, V.S. Eganov, G.G.
Karapetyan; Cosmic Ray Division, Alikhanyan
National Laboratory, Yerevan,
Armenia
13. Median filtering algorithms for multichannel detectors
A. Hovhannisyan, A.
Chilingarian; Cosmic Ray Division,
Alikhanyan National Laboratory, Yerevan, Armenia
14. Variability of Low Energy Cosmic Rays Near Earth
K. Kudela; Institute of Experimental Physics, Slovak Academy of Sciences, Kosice Slovakia
