The GAMMA-1 data on the March 26, 1991 solar flare

Autor:	I. M. Chertok, V. V. Akimov, N. G. Leikov, V. G. Kurt
Rok vydání:	1994
Předmět:	Physics Nuclear physics High energy Pion Solar flare Astrophysics::High Energy Astrophysical Phenomena Physics::Space Physics Bremsstrahlung Electron Plasma Nuclear Experiment Ion Magnetic field
Zdroj:	AIP Conference Proceedings.
ISSN:	0094-243X
Popis:	Two different components of γ‐emission with energies from 30 MeV to several hundred MeV were observed in the solar flare with total duration of 10 minutes. The first, impulsive one, originates as a bremsstrahlung of electrons accelerated at high plasma density (n≳1014 cm−3). The second, delayed component, is associated with a pion production of high energy ions accelerated at low densities in the corona during the stage of magnetic field restoration.
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_________::2de329b1acf048a3a26b4152dda35119 https://doi.org/10.1063/1.45212 Zobrazit plný text záznamu