Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Radiophysical Research Institute, B.Pecherskaya 25, 603950, Nizhny Novgorod, Russia
Max-Planck-Institut fuer Kernphysik, Heidelberg, Germany
Nauchno-Issledovatel'skii Radiofizicheskii Institut, Gorki, USSR
Pulkovo Observatory;, Radiophysical Research Institute
NIRFI, Nizhni Novgorod, 603600, Russia
Pulkovo Astronomical Observatory, Russian Academy of Sciences
CSTR / NJIT
Nobeyama Solar Radio Observatory / NAOJ, Nagano 384-1305, Japan; Central Astronomical Observatory at Pulkovo, Russian Academy of Sciences, St-Petersburg 196140, Russia
Radiophysical Research Institute, 603600 Nizhny Novgorod, Russia
Central Astronomical Observatory at Pulkovo of the Russian Academy of Sciences;, Nobeyama Solar Radio Observatory
Radiophysical Research Institute, 25 Bol'shaya Pecherskaya, 603600 Nizhny Novgorod, Russia
Space Research Institute, Moscow, 117810, RussiaA. V.BelovI. M.ChertokIZMIRAN, Troitsk, Moscow Region, 142092, RussiaV. G.KurtInstitute of Nuclear Physics, Moscow University, Moscow, 119899, RussiaA.MagunInstitute of Applied Physics, University of Bern, CH-3012 Bern, SwitzerlandV. F.MelnikovRadiophys. Research Inst., N.-Novgorod, 603600, Russia
Beijing Astronomical Observatory, National Astromonical Observatoires, Beijing 100012, PR China; Radiophysical Research Institute, 603950 Nizhny Novgorod, Russia MA, US
Moskovskii Gosudarstvennyi Universitet, Moscow; Nauchno-Issledovatel'skii Radiofizicheskii Institut, Gorki, USSR
Radiophysical Research Institute, 25 B. Pecherskaya, 603600 Nizhny Novgorod, Russia
Radiophysical Research Institute, Nizhnii Novgorod 603950, Russia
2002 August 24 Limb Flare Loop: Dynamics of Microwave Brightness Distribution
A Computerized Data Collection and Reduction for Patrol Observations of the Sun in the Centimeter and Decimeter Range
A Microwave Imaging Observation of an Electron Stream in a Solar Flare by Nobeyama Radioheliograph
A New Radio Diagnostic for Razin Suppression
Ballooning Instability in Coronal Flare Loops
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