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• W1986544504 abstract "We have selected four widely different flares from the early period of operations of the Hard X-Ray Imaging Spectrometer (HXIS) on SMM to illustrate the characteristic imaging properties of this experiment. For the small flare of April 4, 1980, we demonstrate the instrument's capability for locating a compact source. In the weak, but extensive, flare of April 6 we show how well the instrument can display spatial structure, and also the low level of the instrument background. In the 1B flare of April 7 we are able to locate positions of the X-ray emission in the soft and hard channels, and estimate the positional variations of the emission patches. Finally, in the IN flare of April 10, which produced the strongest hard X-ray burst we have seen so far, we repeat some of the studies made for the April 7 event, and also demonstrate the capability of the HXIS instrument to study the development, with high time resolution, of individual 8″ × 8″ elements of the flare." @default.
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• W1986544504 date "1981-01-01" @default.
• W1986544504 modified "2023-10-16" @default.
• W1986544504 title "Solar maximum mission experiment: Early results of the hard X-ray imaging experiment" @default.
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• W1986544504 doi "https://doi.org/10.1016/0273-1177(81)90206-4" @default.
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