Hard X-rays in Descent
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Revision as of 09:37, 1 May 2013 by AidanOFlannagain (Talk | contribs)
| Nugget | |
|---|---|
| Number: | 200 |
| 1st Author: | Aidan O'Flannagain |
| 2nd Author: | John Brown and Peter Gallagher |
| Published: | May 6, 2013 |
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Contents |
Electron Beams in the Chromosphere
Figure 1: An illustration of thick target model-based HXR emission in a semicircular flare loop. From top to bottom, the injected spectral index drops from 5 to 4, which results in a descent of peak emission.
Text 1.
Figure 2: Top: Lightcurve of soft (3-6 keV, red) and hard (12-25 keV, blue) X-rays. Also shown is the spectral index of the injected electron distribution (dashed line). Bottom: RHESSI images of 3-6 keV emission, taken at the time indicated by vertical bars in the lightcurve.
Detection of Hard X-rays
Text 2.
Figure 3: Three phase loop lifetime shown by plots of plasma temperature, X-ray emission, loop width/corpulence and thermal pressure for each flare (left:23-Aug-2005, middle:14/15-Apr-2002 and right:21-May-2004). The pattern repeats for the 14/15-Apr-2002 flare due to the multiple X-ray peaks. The shaded orange bars denote each phase.
Explanation
Text 3.
Closer to an Answer
Text 4.
References and links in the article
[1] [http Title]
Acknowledgement.
Facts about Hard X-rays in DescentRDF feed
| RHESSI Nugget Date | 6 May 2013 + |
| RHESSI Nugget First Author | Aidan O'Flannagain + |
| RHESSI Nugget Index | 200 + |
| RHESSI Nugget Second Author | John Brown and Peter Gallagher + |
