The Moon
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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Tethys
September 2013
The shape model of Tethys derived by Robert Gaskell from Cassini Imaging Science Subsystem narrow and wide angle camera (ISSNA and ISSWA) images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on July 25, 2012.
Data
Gaskell Tethys shape Model PDS SBN data archive. September 2013
Publications
Gaskell Tethys Shape Model V1.0
Reference Citation: Gaskell, R.~W.\ 2013.\ Gaskell Tethys Shape Model V1.0.\ NASA Planetary Data System CO-SA-ISSNA-5-TETHYSSHAPE-V1.0.
Abstracts
PDS Gaskell Tethys Shape Model V1.0 NASA Planetary Data System, id. CO-SA-ISSNA-5-TETHYSSHAPE-V1.0Paragraph
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Dione
July 2013
The shape model of Dione derived by Robert Gaskell from Cassini images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on July 23, 2012.
Data
Gaskell Dione shape model PDS SBN data archive September 2013
Publications
Gaskell Dione Shape Model V1.0
Reference Citation: Gaskell, R.~W.\ 2013.\ Gaskell Dione Shape Model V1.0.\ NASA Planetary Data System CO-SA-ISSNA/ISSWA-5-DIONESHAPE-V1.0.
Abstracts
NASA PDS Gaskell Dione Shape Model V1.0 2013 NASA Planetary Data System, id. CO-SA-ISSNA/ISSWA-5-DIONESHAPE-V1.0Paragraph
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Phoebe
August 2012
The shape model of Phoebe derived by Robert Gaskell from Cassini images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on August 4, 2012.
Data
Gaskell Phoebe shape model PDS SBN data archive 2012
Publications
Gaskell Phoebe Shape Model V2.0
Reference Citation: Gaskell, R.~W.\ 2013.\ Gaskell Phoebe Shape Model V2.0.\ NASA Planetary Data System CO-SA-ISSNA-5-PHOEBESHAPE-V2.0.
Abstracts
PDS Gaskell Phoebe shape model paper NASA Planetary Data System, id. CO-SA-ISSNA-5-PHOEBESHAPE-V2.0.
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Mimas
April 2011
The shape model of Mimas derived by Robert Gaskell from Cassini ISSNA images and Voyager 1 ISSN images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on July 14, 2010.
Data
Gaskell Mimas shape model SBN PDS data archive, September 2013
Publications
Gaskell Mimas Shape Model V2.0
Reference Citation: Gaskell, R.~W.\ 2013.\ Gaskell Mimas Shape Model V2.0.\ NASA Planetary Data System CO-SA-ISSNA-5-MIMASSHAPE-V2.0.
Abstracts
NASA PDS Gaskell Mimas Shape Model V2.0 NASA Planetary Data System, id. CO-SA-ISSNA-5-MIMASSHAPE-V2.0Paragraph
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Phobos
March 2006
The shape model of Phobos derived by Robert Gaskell from Viking Orbiter 1 and Phobos 2 images. The model is provided in the implicitly connected quadrilateral (ICQ) format. This version of the model was prepared on March 11, 2006.
Data
Gaskell Phobos shape model PDS SBN data archive, April 2011
Publications
Phobos Shape Model V1.0
Reference Citation: Gaskell, R.~W.\ 2011.\ Phobos Shape Model V1.0.\ NASA Planetary Data System VO1-SA-VISA/VISB-5-PHOBOSSHAPE-V1.0.
Abstracts
NASA PDS “Phobos shape model” Gaskell 2006 NASA Planetary Data System, id. VO1-SA-VISA/VISB-5-PHOBOSSHAPE-V1.0
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