A Study of the 12 June 2010 C6.1/SF flare associated with a CME, surge and energetic particles
Abstract
In this paper, we present the multiwavelength analysis of the C6.1/SF flare on 12 June 2010 from NOAA AR 11081. The flare was observed by various ground based (ARIES H-alpha; HIRAS Radio) and space borne observatories (SDO, STEREO, SOHO, GOES). The flare was accompanied by a spray/surge and a slow coronal mass ejection (CME) that propagated with a speed of ~382 km/s. The eruption was associated with a weak solar energetic particle (SEP) event. The solar source of the eruption was a rapid emerging flux region. The eruption was also associated with the three major types of radio bursts (type II, III and IV). The interesting observation is the shock production (type II burst and SEP event) by a relatively slow CME. We interpret the results in the light of existing theories.
- Publication:
-
39th COSPAR Scientific Assembly
- Pub Date:
- July 2012
- Bibcode:
- 2012cosp...39.2026U