Measurements of excess brightness from solar faculae and the implication for solar oblateness

Details Measurements of excess brightness from solar faculae and the implication for solar oblateness Measurements of excess brightness from solar faculae and the implication for solar oblateness

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975nyasa.262..481c&link_type=abstract

(AAS, American Physical Society, and New York Academy of Sciences, Texas Symposium on Relativistic Astrophysics, 7th, Dallas, Te

Astronomy and Astrophysics

Astrophysics

5

Astronomical Photometry, Brightness Temperature, Faculae, Solar Oblateness, Solar Activity Effects, Solar Flux Density, Solar Limb, Solar Magnetic Field

Scientific paper

Photometric brightness scans were made of the extreme solar limb in an
attempt to show that solar oblateness excess is due to the activity of
faculae. Apparent geometrical oblateness produced by specific facular
regions was observed on 12 of 18 observing days, with the remaining 6
days revealing no oblateness-excess signals.

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