Dark filaments observed at 8.3mm and 3.1mm wavelength

Details Dark filaments observed at 8.3mm and 3.1mm wavelength Dark filaments observed at 8.3mm and 3.1mm wavelength

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986nascp2442..109h&link_type=abstract

In NASA. Goddard Space Flight Center Coronal and Prominence Plasmas p 109-116 (SEE N87-20871 13-92)

Physics

2

Radio Telescopes, Solar Physics, Solar Prominences, Spatial Resolution, Sun, Brightness Temperature, Wavelengths

Scientific paper

Mapping of the sun was made at 3.1mm (98 GHz) and 8.3mm (36 GHz)
wavelengths with a 45m dish radio telescope at the Nobeyama Cosmic Radio
Observatory. The depressions associated with large H alpha filaments are
derived to be -0.2 at 8.3mm and -0.05 at 3.1mm, which are darker than
the values inferred by Raoult et al. (1979)

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