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- W1636162502 abstract "Millimeter‐interferometer observations of flares are used to study the MeV‐energy electrons accelerated in solar flares. The focus of this study is a remarkable similarity found in the time profiles of emission associated with the impulsive onset of a flare. In a large fraction of flares, the impulsive phase emission at millimeter wavelengths consists of a rapid rise (∼5 seconds) linear in time to a sharp peak, followed by an exponential decay with a decay constant of order 15 seconds. The onset of millimeter emission may be delayed by several seconds with respect to the onset of hard X‐rays. The implications of this homologous property are discussed briefly." @default.
- W1636162502 created "2016-06-24" @default.
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- W1636162502 date "1994-01-01" @default.
- W1636162502 modified "2023-09-25" @default.
- W1636162502 title "Energetic electron populations in solar flares" @default.
- W1636162502 doi "https://doi.org/10.1063/1.45191" @default.
- W1636162502 hasPublicationYear "1994" @default.
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