Observations from space of the solar corona/inner zodical light

Details Observations from space of the solar corona/inner zodical light Observations from space of the solar corona/inner zodical light

Dec 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973p%26ss...21.2173m&link_type=abstract

Planetary and Space Science, Volume 21, Issue 12, p. 2173-2173.

Physics

12

Scientific paper

Observations, from the Apollo 16 Spacecraft, in lunar orbit, of the total radiance of the K + F corona, from 3 Rsolar to 55 Rsolar are presented and discussed. The logarithmic slope of the K + F coronal radiance, in the region r > 20 Rsolar, is found to be n = 1.93, slightly less steep than previous determinations. The photometric axis of the radiance is found to be displaced 3 +/- 1° north of the ecliptic, for the region r > 20 Rsolar, and this displacement is interpreted as an annual variation due to non-coincidence of the ecliptic and the symmetry axis of the zodiacal cloud.

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