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Is it possible to model observed active region coronal emission simultaneously in EUV and X-ray filters?

SYSNO ASEP	0364785
Document Type	J - Journal Article
R&D Document Type	Journal Article
Subsidiary J	Článek ve WOS
Title	Is it possible to model observed active region coronal emission simultaneously in EUV and X-ray filters?
Author(s)	Dudík, J. (SK) Dzifčáková, Elena (ASU-R)_{RID, ORCID} Karlický, Marian (ASU-R)_{RID, ORCID} Kulinová, Alena (ASU-R)_{RID, ORCID}
Source Title	Astronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361 Roč. 531, July (2011), A115/1-A115/19
Number of pages	19 s.
Language	eng - English
Country	FR - France
Keywords	Sun corona ; Sun UV radiation ; Sun X-rays
Subject RIV	BN - Astronomy, Celestial Mechanics, Astrophysics
R&D Projects	IAA300030701 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
	GA205/09/1705 GA ČR - Czech Science Foundation (CSF)
	GA205/09/1469 GA ČR - Czech Science Foundation (CSF)
CEZ	AV0Z10030501 - ASU-R (2005-2011)
UT WOS	000293017700029
DOI	10.1051/0004-6361/201015947
Annotation	We investigate the possibility of modeling the active region coronal emission in the EUV and X-ray filters using one, universal, steady heating function, tied to the properties of the magnetic field.
Workplace	Astronomical Institute
Contact	Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2012

Number of the records: 1