Difference between revisions of "Tompkins & Pieters, 1999"
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=Tompkins & Pieters, 1999= | =Tompkins & Pieters, 1999= | ||
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==Description== | ==Description== | ||
The authors use [[Clementine|Clementine]] UVIS multispectral data to characterize the [[Central%20peak%20composition|mineralogical composition]] of the central peaks of 109 impact craters ranging in diameter from 40 to 180 km. These craters can be found by typing the word Tompkins in the search box to the left.<br /> <br /> | The authors use [[Clementine|Clementine]] UVIS multispectral data to characterize the [[Central%20peak%20composition|mineralogical composition]] of the central peaks of 109 impact craters ranging in diameter from 40 to 180 km. These craters can be found by typing the word Tompkins in the search box to the left.<br /> <br /> | ||
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Stefanie Tompkins and Carle M. Pieters (1999) [http://adsabs.harvard.edu/abs/1999M&PS...34...25T Mineralogy of the lunar crust: Results from Clementine] ''Meteoritics & Planetary Science, vol. 34'', pp. 25-41 .<br /> <br /> | Stefanie Tompkins and Carle M. Pieters (1999) [http://adsabs.harvard.edu/abs/1999M&PS...34...25T Mineralogy of the lunar crust: Results from Clementine] ''Meteoritics & Planetary Science, vol. 34'', pp. 25-41 .<br /> <br /> | ||
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Latest revision as of 16:55, 15 April 2018
Contents
Tompkins & Pieters, 1999
(glossary entry)
Description
The authors use Clementine UVIS multispectral data to characterize the mineralogical composition of the central peaks of 109 impact craters ranging in diameter from 40 to 180 km. These craters can be found by typing the word Tompkins in the search box to the left.
Additional Information
LPOD Articles
Bibliography
Stefanie Tompkins and Carle M. Pieters (1999) Mineralogy of the lunar crust: Results from Clementine Meteoritics & Planetary Science, vol. 34, pp. 25-41 .
