NASA NTRS · 19720011145
Analysis of solar X-ray data
Abstract
Type III solar bursts occurring in the absence of solar flares were observed to be accompanied by weak X-radiation. The energy scale of an OSO-3 soft X-ray ion chamber was assessed using realistic theoretical X-ray spectra. Relationships between soft solar X-rays and solar activity were investigated. These included optical studies, the role of the Type III acceleration mechanism in establishing the soft X-ray source volume, H alpha flare intensity variations, and gross magnetic field structure.
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Teske, R. G.. 1972-01-01. Analysis of solar X-ray data. https://ntrs.nasa.gov/citations/19720011145
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