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- W33714892 abstract "The intensity of solar X-radiation scattered by a comet is calculated and compared to the proper X-radiation of the comet due to impacts of cometary and interplanetary dust particles. Detection of X-radiation of dusty comets at small heliocentric distances (R ≤ 1 a. u.) is found to be an indicator of high-temperature plasma generation as result of grain collisions." @default.
- W33714892 created "2016-06-24" @default.
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- W33714892 date "1985-01-01" @default.
- W33714892 modified "2023-09-23" @default.
- W33714892 title "On Two Mechanism OP X-Ray Generation in Comets" @default.
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- W33714892 doi "https://doi.org/10.1007/978-94-009-5464-9_71" @default.
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