The variation of solar brightness at the extreme solar limb at centimetre radio waves

Details The variation of solar brightness at the extreme solar limb at centimetre radio waves The variation of solar brightness at the extreme solar limb at centimetre radio waves

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979soph...63..271l&link_type=abstract

Solar Physics, vol. 63, Sept. 1979, p. 271-274.

Physics

4

Brightness, Centimeter Waves, Solar Limb, Solar Radio Emission, Atmospheric Models, Far Ultraviolet Radiation, Solar Atmosphere, Spicules

Scientific paper

In this note some properties of the nonconvolved brightness profile
close to the extreme solar limb are described. In particular, at 6 cm
and 11 cm wavelength relatively strong, narrow spikes should occur,
noticeably affected by inhomogeneities (for example spicules) in the
solar atmosphere.

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