A method for investigating the brightness distribution near the solar limb at millimeter wavelengths

Details A method for investigating the brightness distribution near the solar limb at millimeter wavelengths A method for investigating the brightness distribution near the solar limb at millimeter wavelengths

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974soph...39..309j&link_type=abstract

Solar Physics, vol. 39, Dec. 1974, p. 309-314.

Physics

3

Brightness Temperature, Limb Darkening, Millimeter Waves, Solar Limb, Astronomical Models, Microwave Emission, Solar Eclipses, Solar Radio Emission

Scientific paper

The brightness distribution near the solar limb has been investigated by means of a technique in which derivatives of drift scans of the sun were compared with derivatives of drift scans of the moon. The results obtained at 88.3 GHz indicate that the sun is limb neutral within the uncertainty of our measurement. If limb brightening or darkening is present, it represents less than 1.6 or 1.2%, respectively, of the total power received from the sun at this wavelength.

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