Measurement of the total luminous flux of the solar corona during sunspot minimum.

Details Measurement of the total luminous flux of the solar corona during sunspot minimum. Measurement of the total luminous flux of the solar corona during sunspot minimum.

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999acaps..19..111z&link_type=abstract

Acta Astrophys. Sin., Vol. 19, No. 1, p. 111 - 112

Astronomy and Astrophysics

Astrophysics

Solar Corona: Solar Activity Cycles, Solar Corona: Sunspots

Scientific paper

The total luminous flux of the solar corona was measured by a photoelectric photometer with a 3° field during the total solar eclipse of 1997 March 9 at Mohe, Heilongjiang Province. The spectral response of the photometer is in accordance with the V(λ) function. The result shows that the relationship between the total luminous flux of the solar corona during sunspot minimum Φc and the total solar luminous flux Φs is Φc = 0.69×10-6Φs.

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