Peculiarities of the surface relief determination by the photoclinometric method in the millimeter range

Author

Dulova, I.A. ; Kornienko, Y.V. ; Skuratovsky, S.I.

Author_Institution

Usikov Inst. of Radiophys. & Electron., NAS Ukraine, Kharkov, Ukraine

Volume

2

fYear

2004

Firstpage

905

Abstract

A method of determination of the relief of a planet surface region by a series of its images is described. It is based on the fact that at given directions of illumination and observation the brightness of a surface element depends on its orientation. Knowing this, one can determine the field of slopes from which it is possible then to reconstruct the relief.

Keywords

astronomical photometry; brightness; covariance matrices; image reconstruction; least squares approximations; millimetre wave imaging; planetary surfaces; radioastronomical techniques; Lambert law; autocovariation matrix; brightness errors; least-squares method; millimeter range; orientation dependence; photoclinometric method; planet surface region; side-looking radar; statistical features; surface element brightness; surface relief determination; Brightness; Density measurement; Extraterrestrial measurements; Image reconstruction; Lighting; Optical surface waves; Planets; Poisson equations; Radar imaging; Surface reconstruction;

fLanguage

English

Publisher

ieee

Conference_Titel

Physics and Engineering of Microwaves, Millimeter, and Submillimeter Waves, 2004. MSMW 04. The Fifth International Kharkov Symposium on

Print_ISBN

0-7803-8411-3

Type

conf

DOI

10.1109/MSMW.2004.1346236

Filename

1346236