Journal
ASTROPHYSICAL JOURNAL LETTERS
Volume 694, Issue 2, Pages L162-L165Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/694/2/L162
Keywords
Sun: flares; Sun: X-rays; gamma rays
Categories
Funding
- NFSC [10773032, 10333030, 10833007]
- 973 program [2006CB806302]
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In this Letter, we studied the time evolution of the energy-dependent spectral indices for the 2004 November 3 solar hard X-ray flare observed by RHESSI. The common soft-hard-soft (SHS) pattern spectra were found at the lower energies, while a new feature, hard-soft-hard (HSH), was found at higher energies for each subpeak. As the energy increases, the SHS pattern is gradually converted into the HSH pattern. Some possible explanations for the spectral evolution and its energy dependence are discussed, such as the return current.
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