Počet záznamů: 1
White-light continuum emission from a solar flare and plage
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SYSNO ASEP 0470168 Druh ASEP C - Konferenční příspěvek (mezinárodní konf.) Zařazení RIV D - Článek ve sborníku Název White-light continuum emission from a solar flare and plage Tvůrce(i) Berlicki, Arkadiusz (ASU-R) RID
Awasthi, A.K. (PL)
Heinzel, Petr (ASU-R) RID, ORCID
Sobotka, Michal (ASU-R) RID, ORCIDZdroj.dok. Solar and Stellar Flares and their Effects on Planets. - Cambridge : Cambridge University Press, 2016 - ISBN 9781107137578 Rozsah stran s. 268-277 Poč.str. 10 s. Forma vydání Tištěná - P Akce Symposium of the International Astronomical Union /320./ Datum konání 11.08.2015 - 14.08.2015 Místo konání Honolulu Země US - Spojené státy americké Typ akce WRD Jazyk dok. eng - angličtina Země vyd. GB - Velká Británie Klíč. slova Sun ; flares ; chromosphere Vědní obor RIV BN - Astronomie a nebeská mechanika, astrofyzika Obor OECD Astronomy (including astrophysics,space science) CEP GA16-18495S GA ČR - Grantová agentura ČR Institucionální podpora ASU-R - RVO:67985815 UT WOS 000452774600044 EID SCOPUS 85054208764 DOI 10.1017/S1743921316002192 Anotace Observations of flare emissions in the optical continuum are very rare. Therefore, the analysis of such observations is useful and may contribute to our understanding of the flaring chromosphere and photosphere. We study the white light continuum emission observed during the X6.9 flare. This emission comes not only from the flare ribbons but also form the nearby plage area. The main aim of this work is to disentangle the flare and plage (facula) emission. We analyzed the spatial, spectral and temporal evolution of the flare and plage properties by analyzing multi-wavelength observations. We study the morphological correlation of the white-light continuum emission observed with different instruments. We found that some active region areas which produce the continuum emission correspond rather to plages than to the flare kernels. We showed that in some cases the continuum emission from the WL flare kernels is very similar to the continuum emission of faculae.
Pracoviště Astronomický ústav Kontakt Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Rok sběru 2017
Počet záznamů: 1