Clementine imagery: Selenographic coverage for cartographic and scientific use

A. C. Cook; J. Oberst; T. Roatsch; R. Jaumann; C. Acton

doi:10.1016/S0032-0633(96)00061-X

Clementine imagery: Selenographic coverage for cartographic and scientific use

A. C. Cook^*, J. Oberst, T. Roatsch, R. Jaumann, C. Acton

^*Corresponding author for this work

Department of Physics

Research output: Contribution to journal › Article › peer-review

40 Citations (Scopus)

Abstract

An investigation is made into the potential use of Clementine imagery for cartographic and scientific studies. A computer search was performed using almost 2 million Clementine image records held on a database at DLR. From this it has been possible to construct maps that illustrate the lunar coverage and height precision of Clementine stereo imagery for stereo mapping. In addition it has been possible to investigate the minimum ground pixel size of multispectral imagery as a function of latitude, and to identify regions where multiple phase angle, and near zero phase angle imagery were obtained.

Original language	English
Pages (from-to)	1135-1148
Number of pages	14
Journal	Planetary and Space Science
Volume	44
Issue number	10 SPEC. ISS.
DOIs	https://doi.org/10.1016/S0032-0633(96)00061-X
Publication status	Published - Oct 1996

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abstract = "An investigation is made into the potential use of Clementine imagery for cartographic and scientific studies. A computer search was performed using almost 2 million Clementine image records held on a database at DLR. From this it has been possible to construct maps that illustrate the lunar coverage and height precision of Clementine stereo imagery for stereo mapping. In addition it has been possible to investigate the minimum ground pixel size of multispectral imagery as a function of latitude, and to identify regions where multiple phase angle, and near zero phase angle imagery were obtained.",

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AB - An investigation is made into the potential use of Clementine imagery for cartographic and scientific studies. A computer search was performed using almost 2 million Clementine image records held on a database at DLR. From this it has been possible to construct maps that illustrate the lunar coverage and height precision of Clementine stereo imagery for stereo mapping. In addition it has been possible to investigate the minimum ground pixel size of multispectral imagery as a function of latitude, and to identify regions where multiple phase angle, and near zero phase angle imagery were obtained.

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Clementine imagery: Selenographic coverage for cartographic and scientific use

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