Soft X-ray heating of the solar chromosphere: gradual phase of a solar flare.

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F02%3A01020184" target="_blank" >RIV/67985815:_____/02:01020184 - isvavai.cz</a>

Result on the web

—

DOI - Digital Object Identifier

—

Result language

angličtina

Original language name

Soft X-ray heating of the solar chromosphere: gradual phase of a solar flare.

Original language description

The authors present the analysis of energetics of solar flaring chromosphete heated by soft X-ray radiation coming from overlying hot flare loops. They show that enhanced emission of some H-alpha structures observed during the gradual phase of this solarflare can be partially explained in terms of the soft X-ray heating of chromosphere.

Czech name

—

Czech description

—

Type

D - Article in proceedings

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

OECD FORD branch

—

Project

—

Continuities

Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year

2002

Confidentiality

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

Article name in the collection

Solar variability: from core to outer frontiers.

ISBN

—

ISSN

—

e-ISSN

—

Number of pages

4

Pages from-to

549-552

Publisher name

ESA Publication Division

Place of publication

Noordwijk

Event location

Praha [CZ]

Event date

Sep 9, 2002

Type of event by nationality

WRD - Celosvětová akce

UT code for WoS article

—