Spectroscopic classification of icy satellites of Saturn I: Identification of terrain units on Dione
• We apply the SAM classification method to 132 infrared VIMS cubes of Dione. • We find nine different spectral units. • We analyze their distribution on the surface of Dione. • We estimate water ice and contaminants abundance variation, and ice grain size. • We compare infrared VIMS spectra of Dion...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Scipioni, F. [verfasserIn] |
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E-Artikel |
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Englisch |
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2013 |
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| Schlagwörter: |
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| Umfang: |
19 |
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| Übergeordnetes Werk: |
Enthalten in: Development of electrophysiological and behavioural measures of electrode discrimination in adult cochlear implant users - Mathew, Rajeev ELSEVIER, 2018, international journal of solar system studies, Orlando, Fla |
|---|---|
| Übergeordnetes Werk: |
volume:226 ; year:2013 ; number:2 ; pages:1331-1349 ; extent:19 |
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| DOI / URN: |
10.1016/j.icarus.2013.08.008 |
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| 520 | |a • We apply the SAM classification method to 132 infrared VIMS cubes of Dione. • We find nine different spectral units. • We analyze their distribution on the surface of Dione. • We estimate water ice and contaminants abundance variation, and ice grain size. • We compare infrared VIMS spectra of Dione and Helene. | ||
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spectroscopic classification of icy satellites of saturn i: identification of terrain units on dione |
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Spectroscopic classification of icy satellites of Saturn I: Identification of terrain units on Dione |
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• We apply the SAM classification method to 132 infrared VIMS cubes of Dione. • We find nine different spectral units. • We analyze their distribution on the surface of Dione. • We estimate water ice and contaminants abundance variation, and ice grain size. • We compare infrared VIMS spectra of Dione and Helene. |
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• We apply the SAM classification method to 132 infrared VIMS cubes of Dione. • We find nine different spectral units. • We analyze their distribution on the surface of Dione. • We estimate water ice and contaminants abundance variation, and ice grain size. • We compare infrared VIMS spectra of Dione and Helene. |
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• We apply the SAM classification method to 132 infrared VIMS cubes of Dione. • We find nine different spectral units. • We analyze their distribution on the surface of Dione. • We estimate water ice and contaminants abundance variation, and ice grain size. • We compare infrared VIMS spectra of Dione and Helene. |
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Spectroscopic classification of icy satellites of Saturn I: Identification of terrain units on Dione |
| url |
https://doi.org/10.1016/j.icarus.2013.08.008 |
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| author2 |
Tosi, F. Stephan, K. Filacchione, G. Ciarniello, M. Capaccioni, F. Cerroni, P. |
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Tosi, F. Stephan, K. Filacchione, G. Ciarniello, M. Capaccioni, F. Cerroni, P. |
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| doi_str |
10.1016/j.icarus.2013.08.008 |
| up_date |
2024-07-06T21:03:21.201Z |
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