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- W2058175926 abstract "Measurements of thermal solar radio noise confirm the existence of a hot corona and indicate the presence of even hotter regions above sunspots. These regions are proposed as a source of coronal energy and their properties investigated. Radio data extending over a period of several years are statistically analysed to separate the total radiation into two components, one associated with sunspots and the other showing no such connection. The following conclusions are reached : ( a ) The sunspot radiation and the very hot regions responsible for it diminish less rapidly than the spot area and exist for a month or more after the spot has vanished. ( b ) For this and other reasons, the non-spot or “ basic component ” at some frequencies is much lower than previously believed. Its actual value is uncertain but it is thought that if spots were absent for many months, most of the radiation would cease. ( c ) This is interpreted as showing that the corona, at least during the period 1947–1951, was mainly due to an agency appearing with sunspots and providing fresh hot gases above the spots. These gases remained after the spots vanished, spreading out to replenish the corona. They appear capable of completely replacing the corona every four days or so." @default.
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- W2058175926 date "1953-10-01" @default.
- W2058175926 modified "2023-09-26" @default.
- W2058175926 title "Thermal Radio Emission from the Sun and the Source of Coronal Heating" @default.
- W2058175926 doi "https://doi.org/10.1093/mnras/113.5.582" @default.
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