A Very Small and Super Strong Zebra Pattern Burst at the Beginning of a Solar Flare
Abstract
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). There is a sudden EUV flash with extra enhancement in one of these FBPs during the ZP burst. Analysis indicates that the ZP burst accompanying an EUV flash is an unusual explosion revealing a strong coherent process with rapid particle acceleration, violent energy release, and fast plasma heating simultaneously in a small region with a short duration just at the beginning of the flare.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- August 2014
- DOI:
- 10.1088/0004-637X/790/2/151
- arXiv:
- arXiv:1406.5209
- Bibcode:
- 2014ApJ...790..151T
- Keywords:
-
- Sun: activity;
- Sun: flares;
- Sun: particle emission;
- Sun: radio radiation;
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- 9 pages, 4 figures, accepted by ApJ