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- W1667483312 abstract "The joint study of hard x ray and microwave observations of solar flares is extremely important because the two complementary ways of viewing the accelerated electrons yield information that cannot be obtained using hard x rays or microwaves alone. The microwaves can provide spatial information lacking in the hard x rays, and the x ray data can give information on the energy distribution of electrons that remove ambiguities in the radio data. A prerequisite for combining the two data-sets, however, is to first understand which range of microwave frequencies correlate best with the hard x rays. This SMM Guest Investigator grant enabled us to combine multi-frequency OVRO data with calibrated hard x ray data to shed light on the relationship between the two emissions. In particular, the questions of which microwave frequencies correspond to which hard x ray energies, and what is the corresponding energy of the electrons that produce both types of emission are investigated." @default.
- W1667483312 created "2016-06-24" @default.
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- W1667483312 date "1992-05-01" @default.
- W1667483312 modified "2023-09-27" @default.
- W1667483312 title "Hard x ray/microwave spectroscopy of solar flares" @default.
- W1667483312 hasPublicationYear "1992" @default.
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