On using the photometric method for a study of Martian topography

Details On using the photometric method for a study of Martian topography On using the photometric method for a study of Martian topography

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978azh....55..419b&link_type=abstract

Astronomicheskii Zhurnal, vol. 55, Mar.-Apr. 1978, p. 419-425. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Photometry, Craters, Mars Surface, Topography, Albedo, Error Analysis, Legendre Functions, Microwaves, Optical Thickness, Planetary Atmospheres, Planetary Surfaces, Reflection, Wavelengths

Scientific paper

The conditions providing a most effective use of the photometric method for determining inclinations on the Martian surface are examined. It is shown that the method works best near the wavelength 0.4 micron. Estimations of the inclinations of exterior and interior walls made for three craters on the surface of Mars gave the following values: 3 to 4 deg for external and 7 to 8 deg for internal walls.

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