Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Akademiia Nauk SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostranenia Radiovoln, Krasnaya Pakhra, USSR
Akademiia Nauk SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Krasnaya Pakhra, USSR
IZMIRAN; National Astronomical Observatoires, Chinese Academy of Sciences
Akademiia Nauk SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Akademgorodok, USSR
AN SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Troitsk, USSR
IZMIRAN, Troitsk, USSR
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radiowave Propagation, Russian Academy of Sciences
IZMIRAN
IZMIRAN, Troitsk, Moscow region, Russia, 142092
IZMIRAN, 142092 Troitsk, Moscow Region, Russia
National Astronomical Observatory, Chinese Academy of Science;, IZMIRAN
National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012; IZMIRAN, Troitsk, Moscow region, 142190, Russia
142092 IZMIRAN, Troitsk, Moscow Region, Russia
IZMIRAN, Moscow, Russia
National Astronomical Observatory, Chinese Academy of Science, 20A, Datun Road, Beijing, 100012, PR China; Izmiran, Troitsk, Moscow region, 142190, Russia SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Akademgorodok, USSR
Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation
IZMIRAN, Akademgorodok, USSR
Akademiia Nauk SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Troitsk, USSR
National Astronomical Observatory, Chinese Academy of Science, 20A, Datun Road, Beijing 100012, PR China; Izmiran Troitsk, Moscow region 142190, Russia
Key Laboratory of Solar Activity, National Astronomical Observatory, Chinese Academy of Science;, IZMIRAN
A Comparative Analysis of Zebra-Pattern Structures at Frequencies from 20 to 7000 MHz
A manifestation of quasilinear diffusion in whistlers in the fine structure of type IV solar radio bursts
A spiky structure of zebra-pattern in solar microwave bursts
A superfine structure in solar microwave bursts
An analysis of fine structures in the range 250 - 450 MHz in a radio burst September, 23, 1998
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