On the structure of filaments from centimeter and millimeter observations

Details On the structure of filaments from centimeter and millimeter observations On the structure of filaments from centimeter and millimeter observations

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...45..125b&link_type=abstract

Solar Physics, vol. 45, Nov. 1975, p. 125-129. Research supported by the Deutsche Forschungsgemeinschaft;

Physics

10

Brightness Temperature, Millimeter Waves, Solar Activity, Bremsstrahlung, Size Determination, Solar Physics, Solar Spectra, Transition Layers

Scientific paper

From filament observations at centimeter and millimeter wavelengths, it is shown that the transition layer between the dense cool filamentary material and the ambient hot rarified corona is rather thin, of the order of some hundred kilometers. Hence, the difference in the sizes of filaments in the radio and optical domains is of the order of 1000 km or 2 sec, thus not detectable by the instruments so far used for observations of filaments.

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