Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Yu. E. Litvinenko"'
Autor:
Yu. E. Litvinenko, Satoshi Masuda, Taro Sakao, E.Y. Merenkova, Sergey A. Bogachev, A. V. Oreshina, Takeo Kosugi, Boris V. Somov
Publikováno v:
Symposium - International Astronomical Union. 203:558-561
On the basis of the Yohkoh data on the site and mechanism of magnetic energy transformation into thermal and kinetic energies of superhot plasmas and accelerated particles, a model is developed that explains observed properties of collisionless 3D re
Autor:
A. Berlicki, A. Minko-Wasiluk, V. V. Akimov, A. V. Belov, I. M. Chertok, P. Ambrož, Marian Karlický, Yu. E. Litvinenko, V. G. Kurt, B. Rompolt, N. G. Leikov, Andreas Magun, Boris V. Somov
Publikováno v:
Scopus-Elsevier
Gamma-ray emission extending to energies greater than 2 GeV and lasting at least for two hours as well as 0.8–8.1 MeV nuclear line emission lasting 40 min were observed with very sensitive telescopes aboard the GAMMA and CGRO satellites for the wel
Autor:
Yu. E. Litvinenko, Boris V. Somov
Publikováno v:
Solar Physics. 158:317-330
Acceleration of protons in a reconnecting current sheet (RCS), which forms as a consequence of filament eruption in the corona, is considered as a possible mechanism of generation of the relativistic particles during the late phase of solar flares. I
Autor:
Yu. E. Litvinenko, Boris V. Somov
Publikováno v:
Solar Physics. 151:265-270
Magnetic reconnection at the photospheric boundary is an essential part of some theories for prominence formation. We consider a simple model for reconnection in this region. Parameters of the reconnecting current sheet are expressed in terms of the
Autor:
Yu. E. Litvinenko
Publikováno v:
Solar Physics. 151:195-198
The reconnecting current sheet model for energy accumulation and release during solar flares results in the flare frequency distribution that is a power-law function of total flare energy, with the index 7/4 for sufficiently large energies. The distr
Autor:
Yu. E. Litvinenko
Publikováno v:
Solar Physics. 147:337-342
Charged particle motion in reconnecting current sheets (CS) can be both regular and chaotic, depending on the values of transverse (perpendicular to the CS plane) and longitudinal (parallel to the electric field inside the CS) components of the magne
Autor:
Yu. E. Litvinenko, Boris V. Somov
Publikováno v:
Solar Physics. 146:127-133
We study motions of charged particles in reconnecting current sheets (CS) which have both transverse (perpendicular to the current sheet plane) and longitudinal (parallel to the electric current inside the sheet) components of the magnetic field. Suc
Autor:
Boris V. Somov, Yu. E. Litvinenko
Publikováno v:
Solar Physics. 131:319-336
The behaviour of the accelerated electrons escaping from a high-temperature source of primary energy in a solar flare is investigated. The direct current of fast electrons is supposed to be balanced by the reverse current of thermal electrons in the
Autor:
Yu. E. Litvinenko, Boris V. Somov
Publikováno v:
Physics of Solar and Stellar Coronae: G.S. Vaiana Memorial Symposium ISBN: 9780792323464
It was believed for a long time and now it is confirmed by Yohkoh observations that magnetic reconnection (i.e., an interaction of magnetic fluxes having pair of antiparallel components) plays a key role in the global dynamics of coronal plasma as we
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dc5f35b66de10fedbb03a0a9d560e260
https://doi.org/10.1007/978-94-011-1964-1_89
https://doi.org/10.1007/978-94-011-1964-1_89