Analysis and modelling of recurrent solar flares observed with Hinode/EIS on March 9, 2012

0479464 - ASÚ 2018 RIV FR eng J - Článek v odborném periodiku
Polito, V. - Del Zanna, G. - Valori, G. - Pariat, E. - Mason, H. E. - Dudík, Jaroslav - Janvier, M.
Analysis and modelling of recurrent solar flares observed with Hinode/EIS on March 9, 2012.
Astronomy & Astrophysics. Roč. 601, May (2017), A39/1-A39/19. ISSN 0004-6361. E-ISSN 1432-0746
Grant CEP: GA ČR GAP209/12/1652; GA ČR(CZ) GA16-17586S
Institucionální podpora: RVO:67985815
Klíčová slova: Sun * flares * UV radiation
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 5.565, rok: 2017

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.
Trvalý link: http://hdl.handle.net/11104/0275458