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- W77836990 abstract "During the summers of 1973 and 1979 the F Corona was observed from ground in the near infrared at 2,2μ and 3,5μ in an attempt to measure the thermal emission peaks predicted by Peterson (1963) and found experi mentally by Peterson (1967) and Mc Queen (1963). These measurements made in solar eclipse time were necessarily short and of limited signal to noise ratio. However they could find emission peaks at 3,4 Ro, 3,9 Ro , 8,7 Ro and 9,2 Ro with the dominant peak at 3.9 Ro. The equivalent width of the peak was of the order of 8 arc. minutes. Different authors have found difficulties to explain the form and the existence of these peaks directly related with the depletion of interplanetary dust falling towards the sun Saito et al (1977) Calbert and Beard (1972) Roser and Stau de (1978). Another authors Mc Queen and Poland (1977), Bohlin (1971) could find coronal brightness changes justifiable by electron streams with long persistence time." @default.
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- W77836990 date "1982-01-01" @default.
- W77836990 modified "2023-09-24" @default.
- W77836990 title "Near Infrared Emission from the Solar Corona" @default.
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- W77836990 doi "https://doi.org/10.1007/978-94-009-7846-1_68" @default.
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