Hard X-ray Patterns of CME-Related Flares
Abstract
The RHESSI hard X-ray spectra are investigated for a total of 23 CME-related flares. It is found that about 17%, 70%, and 13% of the samples can be attributed to type A, B, and C, respectively. These ratios are not significantly different from those obtained using the data of HXRBS/SMM, although the ratio of type C in our CME-related flares is a little higher. More samples are obviously necessary to study the difference of hard X-ray spectra between the CME-related flares and non-CME-related flares.
- Publication:
-
Coronal and Stellar Mass Ejections
- Pub Date:
- 2005
- DOI:
- Bibcode:
- 2005IAUS..226..117L