Problems associated with the transport of energy and acceleration of charged particles in solar flares are considered. Existing theories are compared with observation with a view to either discriminating between rival theories (such as whether hard X-rays are emitted by thermal or nonthermal bremsstrahlung), constraining existing theories (such as deduction of the number of nonthermal electrons present from spectroscopic diagnostics in the soft X-ray part of the spectrum), or suggesting theories (such as attempting to explain the observed spatial structure of microwave emission relative to alpha)
The study of solar activity requires evolutionary and synoptic observations which would be benefitte...
The major results from SMM (Solar Max Mission) are presented as they relate to the understanding of ...
During the period of this contract (February 1 1980 to February 1987) there were two separate effort...
The general objectives of the conference were as follows: (1) Synthesize flare studies after three y...
The proceedings of a symposium of high energy phenomena on the sun are presented. The subjects discu...
The contributions of the High Energy Flare Physics Special Session in the American Astronomical Soci...
The Solar Maximum Mission was used to study solar coronal phenomena in hard X-radiation, since its i...
The results of a NASA science working group established to study a follow-on to the Solar Maximum Mi...
The Science Working Group for the High Resolution Solar Observatory (HRSO) laid plans beginning in 1...
The work of this thesis has been concerned with various aspects of the solar flare phenomenon, and c...
A summary of the proceedings from the workshop are presented. The areas covered were solar activity,...
To address the central scientific questions surrounding solar flares, coordinated observations of el...
A summary of the proceedings of a conference whose purpose was to explore plasma physics problems wh...
The aim of the research activity was to increase our understanding of solar activity through data an...
Observations of the spectral characteristics of solar radio bursts were made with new dynamic spectr...
The study of solar activity requires evolutionary and synoptic observations which would be benefitte...
The major results from SMM (Solar Max Mission) are presented as they relate to the understanding of ...
During the period of this contract (February 1 1980 to February 1987) there were two separate effort...
The general objectives of the conference were as follows: (1) Synthesize flare studies after three y...
The proceedings of a symposium of high energy phenomena on the sun are presented. The subjects discu...
The contributions of the High Energy Flare Physics Special Session in the American Astronomical Soci...
The Solar Maximum Mission was used to study solar coronal phenomena in hard X-radiation, since its i...
The results of a NASA science working group established to study a follow-on to the Solar Maximum Mi...
The Science Working Group for the High Resolution Solar Observatory (HRSO) laid plans beginning in 1...
The work of this thesis has been concerned with various aspects of the solar flare phenomenon, and c...
A summary of the proceedings from the workshop are presented. The areas covered were solar activity,...
To address the central scientific questions surrounding solar flares, coordinated observations of el...
A summary of the proceedings of a conference whose purpose was to explore plasma physics problems wh...
The aim of the research activity was to increase our understanding of solar activity through data an...
Observations of the spectral characteristics of solar radio bursts were made with new dynamic spectr...
The study of solar activity requires evolutionary and synoptic observations which would be benefitte...
The major results from SMM (Solar Max Mission) are presented as they relate to the understanding of ...
During the period of this contract (February 1 1980 to February 1987) there were two separate effort...