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- W2102016041 abstract "The semi-empirical models of the solar chromosphere are useful in the study of the solar radio emission at millimeter - infrared wavelengths. However, current models do not reproduce the observations of the quiet sun. In this work we present a theoretical study of the radiative transfer equation for four semi- empirical models at these wavelengths. We found that the Chromospheric Solar Milimeter- wave Cavity (CSMC), a region where the atmosphere becomes locally optically thin at millimeter wavelengths, is present in the semi- empirical models under study. We conclude that the CSMC is a general property of the solar chromosphere where the semi-empirical models shows temperature minimum.doi: https://doi.org/10.1016/j.gi.2015.04.011" @default.
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- W2102016041 date "2015-04-01" @default.
- W2102016041 modified "2023-10-17" @default.
- W2102016041 title "The Chromospheric Solar Millimeter-wave Cavity; a Common Property in the Semi-empirical Models" @default.
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- W2102016041 doi "https://doi.org/10.1016/j.gi.2015.04.011" @default.
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