Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2011-04-06
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
11 pages, 15 figures; to be published in Astronomy and Astrophysics
Scientific paper
Context: The Yohkoh/HXT observations of Long Duration Events (LDEs) showed that the HXR emission (14-23 keV) is present for tens of minutes after flare maximum. Hence, some heating process is expected to exist during that time. The better energy resolution of RHESSI compared to HXT allow us to analyse LDEs in more comprehensive way. Aims: We selected three LDEs observed by RHESSI to answer the questions how long HXR emission can be present, where it is emitted, what is its nature and how much energy should be released to sustain the emission. Methods: We used RHESSI data to reconstruct images of the selected flares with an energy resolution as good as 1 keV. Next we estimated physical parameters of HXR sources through imaging spectroscopy. The physical parameters obtained were then used to calculate the energy balance of the observed sources. Results: We found that HXR thermal emission can be present for many hours after LDE flare maximum. The emission comes from large and hot loop-top sources. The total energy that must be released to sustain the emission of the sources is as high as 10^31 erg.
Bak-Steslicka Urszula
Kolomanski Sylwester
Mrozek Tomasz
No associations
LandOfFree
RHESSI Observations of Long-Duration Flares With Long-Lasting X-ray Loop-Top Sources does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with RHESSI Observations of Long-Duration Flares With Long-Lasting X-ray Loop-Top Sources, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and RHESSI Observations of Long-Duration Flares With Long-Lasting X-ray Loop-Top Sources will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-418339