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Analysis and modelling of recurrent solar flares observed with Hinode/EIS on March 9, 2012
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SYSNO ASEP 0479464 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title Analysis and modelling of recurrent solar flares observed with Hinode/EIS on March 9, 2012 Author(s) Polito, V. (GB)
Del Zanna, G. (GB)
Valori, G. (GB)
Pariat, E. (FR)
Mason, H. E. (GB)
Dudík, Jaroslav (ASU-R) RID, ORCID
Janvier, M. (GB)Source Title Astronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
Roč. 601, May (2017), A39/1-A39/19Number of pages 19 s. Publication form Online - E Language eng - English Country FR - France Keywords Sun ; flares ; UV radiation Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics OECD category Astronomy (including astrophysics,space science) R&D Projects GAP209/12/1652 GA ČR - Czech Science Foundation (CSF) GA16-17586S GA ČR - Czech Science Foundation (CSF) Institutional support ASU-R - RVO:67985815 UT WOS 000402313500039 EID SCOPUS 85018889982 DOI 10.1051/0004-6361/201629703 Annotation Three homologous C-class flares and one last M-class flare were observed by both the Solar Dynamics Observatory (SDO) and the Hinode EUV Imaging Spectrometer (EIS) in the AR 11429 on March 9, 2012. All the recurrent flares occurred within a short interval of time (less than 4 h), showed very similar plasma morphology and were all confined, until the last one when a large-scale eruption occurred. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2018
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