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- W1504135267 abstract "We attempt to discover whether the emission seen in the Yohkoh HXT-LO (14–24 keV) channel is thermal, due to the presence of high temperature plasma, or nonthermal, as an extension of the nonthermal emission seen at higher energies (>30 keV). We assume that the HXT-LO emission is thermal, and ask: Under what conditions (i.e., T and EM) will a thermal source be consistent with the HXT-LO emission, and the line emission observed by the Yohkoh BCS? All impulsive events, with HXR rise times ranging from 30 seconds to five minutes, observed by Yohkoh are included." @default.
- W1504135267 created "2016-06-24" @default.
- W1504135267 creator A5051791355 @default.
- W1504135267 date "1998-01-01" @default.
- W1504135267 modified "2023-09-24" @default.
- W1504135267 title "Limits on the Temperature of Impulsive Phase Solar Flare Hard X-ray Emission, and the Amount of Thermal X-rays Present in the Yohkoh HXT-LO (14–24 keV) Channel" @default.
- W1504135267 cites W1988881040 @default.
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- W1504135267 doi "https://doi.org/10.1007/978-94-011-5220-4_53" @default.
- W1504135267 hasPublicationYear "1998" @default.
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