Interpretation of millimeter and sub-millimeter observations of the solar chromosphere

Details Interpretation of millimeter and sub-millimeter observations of the solar chromosphere Interpretation of millimeter and sub-millimeter observations of the solar chromosphere

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ijimw...5.1165c&link_type=abstract

(Symposium on Millimetre and Sub-Millimetre Wave Research, Canberra, Australia, Sept. 12-14, 1983) International Journal of Infr

Computer Science

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Brightness Temperature, Chromosphere, Microwave Sounding, Solar Atmosphere, Microwave Interferometers, Millimeter Waves, Solar Limb, Submillimeter Waves

Scientific paper

Solar radiation measurements made in the 100 micron-10 mm spectral range yield data on the variation of brightness temperature with wavelength and disk position that impose important constraints on models of the solar chromosphere structure. Attention is given to relationships explored to date between absolute radiometry and homogeneous models and between center-to-limb variations and inhomogeneous models. It is noted that a 100-m antenna is able to resolve large scale solar structures in the spectral range considered.

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