Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
AN SSSR, Sibirskii Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Irkutsk, USSR
Inst. of Solar-Terrestrial Physics, Irkutsk, Russia
Institute for Solar Terrestrial Physics, Russian Academy of Sciences, Siberian Branch
Sibirskii IZMIRAN, Irkutsk, USSR
Institute of Solar-Terrestrial Physics, P.O. Box 4026, 664033 Irkutsk, Russia
Institute of solar-terrestrial physics SB RAS, P.O. Box 291, 664033, Irkutsk, Russia
Institute of Solar-Terrestrial Physics, Irkutsk, Russia
Institute of Solar-Terrestrial Physics, Siberian Division, Russian Academy of Sciences
Institute of Solar-Terrestrial Physics, Siberian Branch of Russian Academy of Sciences
Institute of Solar-Terrestrial Physics, 664033 Irkutsk, P.O. Box 4026, Russia
Institute of Solar Terrestrial Physics, Russian Academy of Sciences, Siberian Branch
Institute of Solar-Terrestrial Physics, Irkutsk, 664033, P.O. Box 4026, Russia
Russian Academy of Sciences, Inst. of Solar-Terrestrial Physics, Irkutsk, Russia
Institute of Solar-Terrestrial Physics, Russian Academy of Sciences, Siberian Branch
Institute of Solar-Terrestrial Physics RAS SB
Institute of Solar-Terrestrial Physics, Siberian Department, Russian Academy of Sciences, Irkutsk, Russia
Akademiia Nauk SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Irkutsk, USSR
Institute of Solar-Terrestrial Physics, Siberian Branch, Russian Academy of Sciences
An investigation of magnetic fields of solar wind transient disturbances at R = 1 AU and determination of their solar sources
An Investigation of Solar Factors Governing Coronal Mass Ejection Characteristics
An investigation of the large-scale magnetic field variations in the corona prior to and after CME eruptions
An investigation of the magnetic field of Transient Disturbances (TD) at the Earth's orbit, and a determination of solar sources of TD from their characteristics at R = 1 AU
An investigation of the relationship between the magnetic storm Dst-index and different types of solar wind streams
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