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- W1967202337 abstract "We present a morphological description of intense, complex type III-like radio emissions in the frequency range from 1 to 14 MHz. This previously unexplored frequency range, between ground-based and space-based observations, corresponds to the transition region (heliocentric distances from ∼2 to 10 R⊙) between the solar corona and interplanetary medium. The complex type III-like radio emissions, some of which are SA events [Cane et al., 1981], are found to have distinctly different radio signatures above and below ∼7 MHz. Above ∼7 MHz, the radio emissions consists of very rapid frequency-drifting structures with time scales of <16 seconds. Below ∼7 MHz, the radio emissions generally blend into slower frequency-drifting type III-like substructures, with the addition of short-duration very narrowband features that are either very slowly frequency drifting or nondrifting. In addition, there is generally a clear diminution in the radio intensity near 7 MHz." @default.
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- W1967202337 date "1999-02-01" @default.
- W1967202337 modified "2023-09-24" @default.
- W1967202337 title "Complex Type III-like radio emissions observed from 1 to 14 MHz" @default.
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- W1967202337 doi "https://doi.org/10.1029/1998gl900317" @default.
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