RHESSI Observations of Particle Acceleration and Energy Release in an Intense Solar Gamma-Ray Line Flare

By R. Lin, S. Krucker, G. Hurford, David M. Smith, H. Hudson, Gordon D. Holman, Richard A. Schwartz, Brian R. Dennis, G. Share, R. Murphy and 3 more. 2003

428 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/c024d3a8cba477a3bd90fce1ef33bd8e359bfe7e

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. M. Temmer
2. H. Hudson
3. P. Chamberlin
4. V. Petrosian
5. Wei Liu
6. Brian R. Dennis
7. F. Eparvier
8. Astrid Veronig

Citations in the corpus

• Hard X-ray emission from the solar corona (2008, background): “The prototype of this class is the event of 23 July 2002 (Lin et al. 2003; Asai et al. 2006), and the events of 3 November 2003 10 UTC (Veronig et al.”
• Downflow Motions Associated with Impulsive Nonthermal Emissions Observed in the 2002 July 23 Solar Flare (2004, background): “It showed a lot of spectacular features, which have been reported in a number of papers (e.g., Lin et al. 2003), and is famous as the first event in whichg-ray images were successfully obtained (Hurford et al. 2003) with theR uven Fig.”
• Electron Bremsstrahlung Hard X-Ray Spectra, Electron Distributions, and Energetics in the 2002 July 23 Solar Flare (2003, background): “One compelling alternative is that the X-ray emission observed in the early rise phase of the flare (before 00:26:00 UT) is, at least in part, thintarget bremsstrahlung from the corona (Lin et al. 2003).”
• ELECTRON ACCELERATION BY MULTI-ISLAND COALESCENCE (2010, methodology): “Note that X-ray observations show that non-thermal electrons alone carry upwards of 10-50% of the released magnetic field energy (Lin et al. 2003, and references therein).”
• Sixty-five years of solar radioastronomy: flares, coronal mass ejections and Sun–Earth connection (2008, background): “45a) allows to confirm the existence in the onset phase of a coronal non-thermal source inferred from HXR observations and which contains a large amount of energy (Lin et al. 2003; Holman et al. 2003; White et al. 2003).”
• A MAGNETIC RECONNECTION MECHANISM FOR ION ACCELERATION AND ABUNDANCE ENHANCEMENTS IN IMPULSIVE FLARES (2009, background): “A significant fraction of this released energy is transferred to energetic electrons and ions, with ions reaching energies in the range of GeV (Lin et al. 2003; Emslie et al. 2004).”
• An Observational Overview of Solar Flares (2011, background): “8) (Lin et al. 2003).”
• Recent Advances in Understanding Particle Acceleration Processes in Solar Flares (2011, methodology): “RHESSIobservations have also provided important information on the temporal evolution of prompt gamma-ray lines (Lin et al. 2003).”