Correlative Analysis of Hard and Soft X-ray Emissions in Solar Flares

Details Correlative Analysis of Hard and Soft X-ray Emissions in Solar Flares Correlative Analysis of Hard and Soft X-ray Emissions in Solar Flares

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997arc..rept.....z&link_type=abstract

Technical Report, Applied Research Corp. Landover, MD United States

Computer Science

Solar Flares, Emission Spectra, X Rays, X Ray Telescopes, Gamma Ray Bursts, Bragg Angle, Observatories, Japanese Spacecraft, Gamma Ray Observatory

Scientific paper

This report describes research performed under the Phase 3 Compton Gamma-Ray Observatory (CGRO) Guest Investigator Program. The objective of this work is to study different mechanisms of solar flare heating by comparing their predictions with simultaneous hard and soft X-ray observations. The datasets used in this work consist of hard X-ray observations from the CGRO Burst and Transient Source Experiment (BATSE) and soft X-ray observations from the Bragg Crystal Spectrometer (BCS) and Soft X-ray telescope (SXT) on the Japanese Yohkoh spacecraft.

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