V. E. Shaposhnikov
University High School
29 Papers
57 Citations
V. E. Shaposhnikov is an academic researcher from University High School. The author has contributed to research in topics: Jovian & Ionosphere. The author has an hindex of 6, co-authored 21 publications. Previous affiliations of V. E. Shaposhnikov include Russian Academy of Sciences & National Research University – Higher School of Economics.
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Papers
Quasi-similar decameter emission features appearing in the solar and jovian dynamic spectra
G. Litvinenko,V. E. Shaposhnikov,A. A. Konovalenko,V. V. Zakharenko,Mykhaylo Panchenko,V. V. Dorovsky,A. I. Brazhenko,Helmut O. Rucker,V. V. Vinogradov,Valentin Melnik +9 more
TL;DR: In this paper, the authors investigate the dynamic spectra of the Sun and jovian decametric radiation obtained by the authors with the radio telescopes UTR-2 and URAN-2 (Kharkov, Poltava, Ukraine).
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•Journal Article
The origin of S-bursts in Jupiter's decametric radio spectra
TL;DR: In this article, a modele des sursauts S, dependant de la phase d'Io, dans l'emission radiodecametrique de Jupiter, is proposed.
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Parametric mechanism for the formation of Jovian millisecond radio bursts
V. E. Shaposhnikov,S. V. Korobkov,Helmut O. Rucker,Alexander Kostrov,Mikhail Gushchin,G. Litvinenko +5 more
TL;DR: In this paper, the formation of a fine structure in the dynamic spectra of the Jovian decametric radio emission was studied, and it was shown that nonstationary disturbances of the planetary magnetic field and the strong frequency dispersion of the plasma at frequencies close to the cutoff frequency of the extraordinary wave in the jovian ionosphere play a crucial role in formation of narrowband emission and quasiperiodic trains of short (S) bursts.
12
Zebra pattern in decametric radio emission of Jupiter
Mykhaylo Panchenko,S. Rošker,Helmut O. Rucker,A. Brazhenko,Philippe Zarka,Philippe Zarka,G. Litvinenko,V. E. Shaposhnikov,Alexandr A. Konovalenko,Valentin Melnik,A.V. Franzuzenko,J. Schiemel +11 more
TL;DR: In this article, a systematic analysis of zebra-like fine spectral structures in decametric frequency range of Jovian radio emission was performed by the large ground-based radio telescope URAN-2 during three observation campaigns between, Sep., 2012 and May, 2015.
12
On ultraviolet emission observed on the flanks of Io
TL;DR: In this paper, the authors proposed the mechanism that provides the sufficient energy of the equatorial spots to explain their high brightness in the UV wavelength range, which is generated due to electrons which are formed as a result of additional ionization of the atmosphere in the front part of the satellite.
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