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Solar limb brightening at 3.1 cm |
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| Authors: | M. Felli G. Tofani |
| Affiliation: | (1) Osservatorio Astrofisico di Arcetri, Italy |
| Abstract: | The existence of limb brightening at the equator of the quiet Sun at 3.1 cm is derived from a statistical analysis of scans of the solar disk taken during 1968.A ratio of 0.7% is found between the flux emitted by the equatorial limb enhancements and that of a disk of uniform brightness temperature. |
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