This report describes work performed under contract NAS5-32584 for Phase 3 of the Compton Gamma Ray Observatory (CGRO) from 1 November 1993 through 1 November 1994. We have made spectral observations of the hard x-ray and gamma-ray bremsstrahlung emissions from solar flares using the Burst and Transit Source Experiment (BASTE) on CGRO. These measurements of their spectrum and time profile provided valuable information on the fundamental flare processes of energy release, particle acceleration, and energy transport. Our scientific objective was to study both the thermal and non-thermal sources of solar flare hard x-ray and gamma-ray emission
The work of this thesis has been concerned with various aspects of the solar flare phenomenon, and c...
One of our primary accomplishments under grant NAGW-35381 was the systematic derivation and compilat...
The work of this thesis has been concerned with various aspects of the solar flare phenomenon, and c...
This report describes research performed under the Phase 3 Compton Gamma-Ray Observatory (CGRO) Gues...
This final report describes the progress originally proposed: (1) the continued improvement of a sof...
The objective of this work is to study different mechanisms of solar flare heating by comparing thei...
The objective of this project is to determine the characteristics of flare energy transport processe...
The 1991 November 15 X1.5 flare was a well observed solar event. Comprehensive data from ground-base...
The X-ray and gamma-ray emission from solar flares provides important information about high-energy ...
The X-ray and gamma-ray emission from solar flares provides important information about high-energy ...
The research performed under this contract is part of an on-going investigation to explore the fines...
This dissertation expands the current understanding of the 15 November 1991 X1.5 solar flare. This f...
A list of publications resulting from this program includes 'The Timing of Electron Beam Signatures ...
We conduct a wide-band X-ray spectral analysis in the energy range of 1.5-100 keV to study the time ...
This work expands the current understanding of the 15 November 1991 Solar Flare. The flare was a wel...
The work of this thesis has been concerned with various aspects of the solar flare phenomenon, and c...
One of our primary accomplishments under grant NAGW-35381 was the systematic derivation and compilat...
The work of this thesis has been concerned with various aspects of the solar flare phenomenon, and c...
This report describes research performed under the Phase 3 Compton Gamma-Ray Observatory (CGRO) Gues...
This final report describes the progress originally proposed: (1) the continued improvement of a sof...
The objective of this work is to study different mechanisms of solar flare heating by comparing thei...
The objective of this project is to determine the characteristics of flare energy transport processe...
The 1991 November 15 X1.5 flare was a well observed solar event. Comprehensive data from ground-base...
The X-ray and gamma-ray emission from solar flares provides important information about high-energy ...
The X-ray and gamma-ray emission from solar flares provides important information about high-energy ...
The research performed under this contract is part of an on-going investigation to explore the fines...
This dissertation expands the current understanding of the 15 November 1991 X1.5 solar flare. This f...
A list of publications resulting from this program includes 'The Timing of Electron Beam Signatures ...
We conduct a wide-band X-ray spectral analysis in the energy range of 1.5-100 keV to study the time ...
This work expands the current understanding of the 15 November 1991 Solar Flare. The flare was a wel...
The work of this thesis has been concerned with various aspects of the solar flare phenomenon, and c...
One of our primary accomplishments under grant NAGW-35381 was the systematic derivation and compilat...
The work of this thesis has been concerned with various aspects of the solar flare phenomenon, and c...