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Observations and modeling of the ultraviolet emission of solar flares

SYSNO ASEP	0470174
Document Type	C - Proceedings Paper (int. conf.)
R&D Document Type	Conference Paper
Title	Observations and modeling of the ultraviolet emission of solar flares
Author(s)	Mikula, K. (PL) Berlicki, Arkadiusz (ASU-R)_RID Heinzel, Petr (ASU-R)_{RID, ORCID}
Source Title	Solar and Stellar Flares and their Effects on Planets. - Cambridge : Cambridge University Press, 2016 - ISBN 9781107137578
Pages	s. 57-59
Number of pages	3 s.
Publication form	Print - P
Action	Symposium of the International Astronomical Union /320./
Event date	11.08.2015 - 14.08.2015
VEvent location	Honolulu
Country	US - United States
Event type	WRD
Language	eng - English
Country	GB - United Kingdom
Keywords	Sun ; chromosphere ; transition region
Subject RIV	BN - Astronomy, Celestial Mechanics, Astrophysics
OECD category	Astronomy (including astrophysics,space science)
Institutional support	ASU-R - RVO:67985815
UT WOS	000452774600005
EID SCOPUS	85054262594
DOI	10.1017/S174392131600048X
Annotation	In this paper we present the method of using far UV spectra of the flare observed by Interface Region Imaging Spectrograph (IRIS) for determination of the contribution of the continuum emission to the total UV radiation observed e.g. by SDO in 1600 Å channel. In our method the Si IV (1402.77 Å) line observed by IRIS is used as a proxy of C IV line emission contained in SDO/AIA UV images. Determined intensity of the flare continuum emission can be used to study the physics of the flare heated chromosphere and for better understanding of the emission mechanisms.
Workplace	Astronomical Institute
Contact	Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2017

Number of the records: 1