A Very Small and Super Strong Zebra Pattern Burst at the Beginning of a Solar Flare

0433653 - ASÚ 2015 RIV US eng J - Článek v odborném periodiku
Tan, B.-L. - Tan, C.M. - Zhang, Y. - Huang, J. - Mészárosová, Hana - Karlický, Marian - Yan, Y.
A Very Small and Super Strong Zebra Pattern Burst at the Beginning of a Solar Flare.
Astrophysical Journal. Roč. 790, č. 2 (2014), 151/1-151/6. ISSN 0004-637X. E-ISSN 1538-4357
Grant CEP: GA ČR GAP209/12/0103
Institucionální podpora: RVO:67985815
Klíčová slova: Sun: activity * Sun: flares * Sun: particle emission
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
Impakt faktor: 5.993, rok: 2014

Microwave emission with spectral zebra pattern structures (ZPs) is frequently observed in solar flares and the Crab pulsar. The previous observations show that ZP is a structure only overlapped on the underlying broadband continuum with slight increments and decrements. This work reports an unusually strong ZP burst occurring at the beginning of a solar flare observed simultaneously by two radio telescopes located in China and the Czech Republic and by the EUV telescope on board NASA's satellite Solar Dynamics Observatory on 2013 April 11. It is a very short and super strong explosion whose intensity exceeds several times that of the underlying flaring broadband continuum emission, lasting for just 18 s. EUV images show that the flare starts from several small flare bursting points (FBPs).
Trvalý link: http://hdl.handle.net/11104/0237842