Response of optical hydrogen lines to beam heating. I. Electron beams

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F09%3A00334858" target="_blank" >RIV/67985815:_____/09:00334858 - isvavai.cz</a>

Alternative codes found

RIV/44555601:13440/09:00004873

Result on the web

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DOI - Digital Object Identifier

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Result language

angličtina

Original language name

Response of optical hydrogen lines to beam heating. I. Electron beams

Original language description

We investigate the role of non-thermal electrons in the formation regions of H?, H?, and H? lines in order to unfold their influence on the formation of these lines. We concentrate on pulse-beam heating varying on a subsecond timescale. Furthermore, we theoretically explore possibility that a new diagnostic tool exists indicating the presence of non-thermal electrons in the flaring chromosphere based on observations of optical hydrogen lines.

Czech name

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Czech description

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Type

J_x - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

OECD FORD branch

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Project

Result was created during the realization of more than one project. More information in the Projects tab.

Continuities

Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year

2009

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Name of the periodical

Astronomy and Astrophysics

ISSN

0004-6361

e-ISSN

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Volume of the periodical

499

Issue of the periodical within the volume

3

Country of publishing house

FR - FRANCE

Number of pages

12

Pages from-to

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UT code for WoS article

000266730600033

EID of the result in the Scopus database

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