Inversion of the zodiacal brightness integral for an out-of-ecliptic photometer

Details Inversion of the zodiacal brightness integral for an out-of-ecliptic photometer Inversion of the zodiacal brightness integral for an out-of-ecliptic photometer

May 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978cosp.meetr....d&link_type=abstract

COSPAR, Plenary Meeting, 21st, Innsbruck, Austria, May 29-June 10, 1978, Paper. 5 p.

Astronomy and Astrophysics

Astronomy

Astronomical Photometry, Celestial Reference Systems, Photometers, Zodiacal Light, Brightness, Ecliptic, Inversions, Rotating Bodies, Stellar Motions, Symmetry

Scientific paper

The paper determines in which viewing directions the photometric data expected from an out-of-ecliptic zodiacal light experiment will allow the inversion of the brightness integral. The minimum assumption is made that the zodiacal cloud has rotational symmetry. If this assumption is correct, many new results on the local optical properties of the interplanetary grains can be expected.

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