Magnetic fields and thermodynamical conditions in the M6.4/3N solar flare on July 19, 2000

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Кинематика и физика небесных тел
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Кинематика и физика небесных тел, 2005 (том 21)
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Кинематика и физика небесных тел, 2005, № 5-додаток
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dc.contributor.author	Kurochka, E.V.
dc.contributor.author	Lozitsky, V.G.
dc.date.accessioned	2015-04-03T16:31:07Z
dc.date.available	2015-04-03T16:31:07Z
dc.date.issued	2005
dc.identifier.citation	Magnetic fields and thermodynamical conditions in the M6.4/3N solar flare on July 19, 2000 / E.V. Kurochka, V.G. Lozitsky // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 143-145. — Бібліогр.: 8 назв. — англ.	uk_UA
dc.identifier.issn	0233-7665
dc.identifier.uri	http://dspace.nbuv.gov.ua/handle/123456789/79627
dc.description.abstract	We present the semi-empirical model of a powerful solar flare on July 19, 2000 based on spectral observations in the Fe I, Fe II, Cr I, and Ti II lines. Our calculations show the existence of a very narrow (≤ 100 km) and sharp magnetic field peak at photospheric level (log τ5 ≈ −2). It is possible that this peculiarity is indicative of the local magnetic field amplification due to specific process during the flare. Yet another interesting detail of the model is two discrete hot flare layers related to the middle photosphere and temperature minimum zone.	uk_UA
dc.description.sponsorship	We are very grateful to Dr. E. A. Baranovsky for placing his program at our disposal.	uk_UA
dc.language.iso	en	uk_UA
dc.publisher	Головна астрономічна обсерваторія НАН України	uk_UA
dc.relation.ispartof	Кинематика и физика небесных тел
dc.subject	MS2: Physics of Solar Atmosphere	uk_UA
dc.title	Magnetic fields and thermodynamical conditions in the M6.4/3N solar flare on July 19, 2000	uk_UA
dc.type	Article	uk_UA
dc.status	published earlier	uk_UA