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• W1488406218 abstract "Estimates from hard X-ray measurements show that for many flares the bulk of the flare energy is released in the form of approximately 10-100-keV energy electrons. The interaction of these electrons with the solar atmosphere can produce the optical, UV, EUV, and radio emissions observed during the flare impulsive phase. In addition, explosive heating and evaporation of the chromosphere by these electrons can produce the roughly 10 million K soft X-ray plasma. For the large solar flares which produce interplanetary shock waves, the accelerated approximately 10-100-keV electron population may produce the heating and mass motion required for mass ejection and the formation of the shock wave. The shock wave can in turn accelerate ions and electrons to higher energy as it travels through the corona and interplanetary medium." @default.
• W1488406218 created "2016-06-24" @default.
• W1488406218 creator A5091566288 @default.
• W1488406218 date "1977-01-01" @default.
• W1488406218 modified "2023-09-23" @default.
• W1488406218 title "Energetic solar flare particles and interplanetary shock waves" @default.
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• W1488406218 doi "https://doi.org/10.1007/978-90-277-0860-1_2" @default.
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