Mathilde

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Stooke shape model (left). Near Image (center). SPC shape model (Right).

Topography of the lunar poles, constructed using stereophotoclinometry (SPC) and Clementine images, is compared with results from LOLA and LRO wide-angle camera analyses.

Publications

Digital Terrain Models of Mathilde and the Moon

Reference Citation: Weirich, J.~R., Palmer, E.~E., Domingue, D.~L.\ 2019.\ Digital Terrain Models of Mathilde and the Moon.\ Lunar and Planetary Science Conference 2681.

Abstracts

https://ui.adsabs.harvard.edu/abs/2011LPI….42.2535G/abstract 50th Lunar and Planetary Science Conference, held 18-22 March, 2019 at The Woodlands, Texas. LPI Contribution No. 2132, id.2681

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The Moon

A comparison of a LROC image to and SPC model of the lunar surface. A 5×5 km subsection of Karpinskiy regional DTM with grid overlay.

Topography of the lunar poles, constructed using stereophotoclinometry (SPC) and Clementine images, is compared with results from LOLA and LRO wide-angle camera analyses.

Publications

Digital Terrain Models of Mathilde and the Moon

Reference Citation: Weirich, J.~R., Palmer, E.~E., Domingue, D.~L.\ 2019.\ Digital Terrain Models of Mathilde and the Moon.\ Lunar and Planetary Science Conference 2681.

Abstracts

https://ui.adsabs.harvard.edu/abs/2011LPI….42.2535G/abstract 50th Lunar and Planetary Science Conference, held 18-22 March, 2019 at The Woodlands, Texas. LPI Contribution No. 2132, id.2681

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