Integral photometry of Mars

Details Integral photometry of Mars Integral photometry of Mars

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978avest..11..137a&link_type=abstract

(Astronomicheskii Vestnik, vol. 11, July-Sept. 1977, p. 137-143.) Solar System Research, vol. 11, no. 3, Jan. 1978, p. 114-119.

Astronomy and Astrophysics

Astronomy

Astronomical Photometry, Brightness, Dust Storms, Electrophotometry, Mars Surface, Light Curve, Phase Deviation, Reference Stars, Stellar Magnitude, Tables (Data)

Scientific paper

Mars was studied via integral photoelectric photometry during a period from August 1975 to January 1976 in the spectral region of 336-798 nm. Peculiarities in the change of brightness during August and September 1975 suggest that a global dust storm took place during that period. Previous observations, obtained from 1954 to 1975, have been used to determine the average phase dependence of the integral brightness of Mars.

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