JPL Technical Report Server
Silicate cooling model fits to Galileo NIMS data of volcanism on IO
- JPL TRS Home
- →
- JPL Technical Report Server
- →
- JPL TRS 1992+
- →
- View Item
JavaScript is disabled for your browser. Some features of this site may not work without it.
| dc.contributor.author | Davies, A. | en_US |
| dc.contributor.author | Lopes-Gautier, R. | en_US |
| dc.contributor.author | Smythe, W. | en_US |
| dc.contributor.author | Carlson, R. | en_US |
| dc.date.accessioned | 2004-09-23T21:10:16Z | |
| dc.date.available | 2004-09-23T21:10:16Z | |
| dc.date.issued | 2000-11 | en_US |
| dc.identifier.citation | Icarus, v. 148, no. 1, pp.211-225 | en_US |
| dc.identifier.citation | Pasadena, CA, USA | en_US |
| dc.identifier.clearanceno | 00-1626 | en_US |
| dc.identifier.uri | http://hdl.handle.net/2014/15852 | |
| dc.description.abstract | The Near Infrared Mapping Spectrometer (NIMS) has obtained spectra of volcanoes on the surface of the jovian satellite Io. | en_US |
| dc.format.extent | 322652 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.language.iso | en_US | |
| dc.subject.other | Thermal emission lava flow active volcanism sulfur flow | en_US |
| dc.title | Silicate cooling model fits to Galileo NIMS data of volcanism on IO | en_US |
Files in this item
This item appears in the following Collection(s)
-
JPL TRS 1992+
JPL TRS 1992+