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Sunquakes: Seismic Transients from Solar Flares
2006-05-08 • submitted by Charlie Lindsey and Alina Donea
26
Observations of large RHESSI flares show that the location of impulsive hard X-rays matches that of the source of sunquake waves.
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Return currents and soft-hard-soft spectral evolution
2006-04-24 • submitted by Valentina Zharkova and Mykola Gordovskyy
25
Self-induced electric fields and return currents explain the soft-hard soft spectral evolution seen in flares.
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Three is company
2006-04-10 • submitted by Marina Battaglia
24
A coronal source shows a soft-hard-soft spectral behavior.
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Birth of a dense flaring loop
2006-03-27 • submitted by Laura Bone
23
The simplest explanations for RHESSI coronal sources is an enhanced coronal density. A discussion of such an interpretation for the 14th April 2002 flare.
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Time delay between HXR and Gamma-rays
2006-03-13 • submitted by Cyril Dauphin and Nicole Vilmer
22
An exploration of a trap and precipitation model to explain the observed time delay between gamma-rays and X-rays in the July 23rd event.
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This material is based upon work supported by NASA unless otherwise noted. Any opinions, findings, and conclusions or recommendations expressed are those of the author(s).