Observations and modeling of the ultraviolet emission of solar flares

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F16%3A00470174" target="_blank" >RIV/67985815:_____/16:00470174 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1017/S174392131600048X" target="_blank" >http://dx.doi.org/10.1017/S174392131600048X</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1017/S174392131600048X" target="_blank" >10.1017/S174392131600048X</a>

Result language
angličtina
Original language name
Observations and modeling of the ultraviolet emission of solar flares
Original language description
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. n
Czech name
—
Czech description
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Project
—
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2016
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
Solar and Stellar Flares and their Effects on Planets
ISBN
9781107137578
ISSN
—
e-ISSN
—
Number of pages
3
Pages from-to
57-59
Publisher name
Cambridge University Press
Place of publication
Cambridge
Event location
Honolulu
Event date
Aug 11, 2015
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000452774600005

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