Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow, Russia
Solar-Terrestrial Center of Excellence, SIDC, Royal Observatory of Belgium, Avenue Circulaire 3, B-1180 Brussels, Belgium ; Skobeltsyn Institute of Nuclear Physics, Moscow State University, 119992 Moscow, Russia
Solar-Terrestrial Center of Excellence, SIDC, Royal Observatory of Belgium, Brussels, Belgium
Solar-Terrestrial Center of Excellence - SIDC, Royal Observatory of Belgium; Skobeltsyn Institute of Nuclear Physics, Moscow State University
Royal Observatory of Belgium, Avenue Circulaire 3, 1180 Brussels, Belgium ; Skobeltsyn Institute of Nuclear Physics, Moscow State University, 119992 Moscow, Russia Observatory of Belgium, Avenue Circulaire 3, Brussels, Belgium - Royal Observatory of Belgium, Av. Circulaire 3, Brussels, 1180, Belgium Observatory of Belgium, Avenue Circulaire 3, B-1180 Brussels, Belgium; Institute of Nuclear Physics, Moscow State University, Moscow 119992, Russia
Solar-Terrestrial Center of Excellence-SIDC, Royal Observatory of Belgium, Avenue Circulaire 3, B-1180 Brussels, Belgium; Skobeltsyn Institute of Nuclear Physics, Moscow State University, 119992 Moscow, Russia
Max-Planck-Institut für Aeronomie, Katlenburg Lindau, Germany
Institute of Nuclear Physics, Moscow State University, 119899 Moscow, Russia
Skobel'tsyn Institute of Nuclear Physics, Moscow State University;, Observatoire Royal de Belgique
Solar-Terrestrial Center of Excellence-SIDC, Royal Observatory of Belgium, Avenue Circulaire 3, B-1180 Brussels, Belgium; Skobeltsyn Institute of Nuclear Physics, Moscow State University, 119992 Moscow, Russia.
Solar - Terrestrial Center of Excellence - SIDC, Royal Observatory of Belgium; Sk
A Year Later: Solar, Heliospheric, and Magnetospheric Disturbances in November 2004
Coronal plasmoid dynamics. I. Dissipative MHD approach
Coronal plasmoid dynamics. II. The nonstationary fine structure
Coronal Seismology Using EIT Waves: Estimation of the Coronal Magnetic Field Strength in the Quiet Sun
Correction to ``Major geomagnetic storms (Dst <= -100 nT) generated by corotating interaction regions''
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