Zobrazeno 1 - 10
of 132
pro vyhledávání: '"Dennis L. Matson"'
Autor:
Torrence V. Johnson, Thomas B. McCord, Jean-Philippe Combe, Federico Tosi, Francesca Scipioni, Ashley Davies, Dennis L. Matson
Publikováno v:
Icarus. 317:491-508
We present the first map of CO2 at the surface of Enceladus using data obtained by the Cassini Visible-Infrared Mapping Spectrometer (VIMS). In order to measure the weak and narrow CO2 absorption band depths around 4.26 µm, we improved: (1) the cali
Autor:
Jani Radebaugh, Torrence V. Johnson, Thomas B. McCord, Dennis L. Matson, Sandeep Singh, Ashley Davies, Jean-Philippe Combe
Publikováno v:
Icarus. 302:18-26
Solid CO2 surface deposits were reported in Enceladus’ South Polar Region by Brown et al. (2006). They noted that such volatile deposits are temporary and posited ongoing replenishment. We present a model for this replenishment by expanding on the
Publikováno v:
Icarus. 274:23-32
To date, there has been no conclusive observation of ongoing endogenous volcanic activity on Saturn's moon Titan. However, with time, Titan's atmospheric methane is lost and must be replenished. We have modeled one possible mechanism for the replenis
Autor:
Sebastien Rodriguez, Bernd Giese, Robert H. Brown, T. Roatsch, Roland Wagner, Cristina M. Dalle Ore, Dale P. Cruikshank, Kevin H. Baines, Phil D. Nicholson, Dennis L. Matson, Roger N. Clark, Bonnie J. Buratti, Fabrizio Capaccioni, Ralf Jaumann, Norbert Krupp, Katrin Stephan, Gianrico Filacchione
Publikováno v:
Icarus
Icarus, 2016, 274, pp.1-22. ⟨10.1016/j.icarus.2016.03.002⟩
Icarus, 2016, 274, pp.1-22. ⟨10.1016/j.icarus.2016.03.002⟩
The Saturnian satellite Tethys exhibits geological and spectral properties, whose appearance, nature and spatial distribution partly mirror those identified on the neighboring satellites Dione and Rhea or fit to the picture how spectral surface prope
Publikováno v:
Icarus. 262:67-78
We present a map of Io’s volcanic heat flow. Io’s high heat flow is a result of intense tidal heating, which generates widespread volcanic activity. The surface expression of ongoing volcanic activity constrains the location and magnitude of tida
Autor:
Torrence V. Johnson, A. G. Davies, I. de Pater, Lionel Wilson, R. L. Davies, Dennis L. Matson, Glenn J. Veeder, K. de Kleer
Analysis of Galileo Near Infrared Mapping Spectrometer (NIMS) observations of Marduk Fluctus, a volcano on the jovian moon Io, reveals a style of volcanic activity not previously seen there – a powerful thermal event lasting only a few minutes in 1
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d6b95b94888cc82d112a67d0d443db39
https://resolver.caltech.edu/CaltechAUTHORS:20190424-103159776
https://resolver.caltech.edu/CaltechAUTHORS:20190424-103159776
Autor:
Jani Radebaugh, Dennis L. Matson, David A. Williams, Ashley Davies, Torrence V. Johnson, Glenn J. Veeder
Publikováno v:
Icarus. 245:379-410
We identify nine new faint thermal sources on Io via color ratio images constructed from relatively high spatial resolution Galileo NIMS data acquired late in the mission. All of these identifications are associated with small dark paterae. We utiliz
Autor:
Chad Trujillo, Ashley Davies, Glenn J. Veeder, Máté Ádámkovics, Alistair McGregor, Giovanni Leone, Imke de Pater, Dennis L. Matson
Publikováno v:
Icarus. 242:379-395
We have imaged Io in the near-infrared (1–5 μm) with adaptive optics on the 10-m W.M. Keck II and the Gemini North telescopes. We have constructed global maps from the data taken in 2010. Although numerous hot spots are visible, the maps are domin
Publikováno v:
Icarus. 241:190-199
We have examined the variability of thermal emission from lava flows at Amirani on Io, using measurements of radiant flux from detections by the Galileo Near Infrared Mapping Spectrometer (NIMS) between 1996 and 2001. Amirani is the longest currently
Autor:
Dale P. Cruikshank, Angioletta Coradini, F. Leader, Pierre Drossart, Karl L. Mitchell, P. Cerroni, Robert M. Nelson, Randolph L. Kirk, Dennis L. Matson, Stephen D. Wall, Fabrizio Capaccioni, John C. Pearl, Kevin H. Baines, Vito Mennella, M. Combes, P. D. Nicholson, Gianrico Filacchione, M. D. Boryta, Ralf Jaumann, L. W. Kamp, Yves Langevin, Rosaly M. C. Lopes, Bruno Sicardy, Thomas B. McCord, Jonathan I. Lunine, Vittorio Formisano, Jean-Pierre Bibring, Roger N. Clark, Bruce Hapke, Patrick G. J. Irwin, Christophe Sotin, Giancarlo Bellucci, William D. Smythe
Publikováno v:
Geophysical Research Letters
Geophysical Research Letters, 2009, 36, pp.04202. ⟨10.1029/2008GL036206⟩
Geophysical Research Letters, 2009, 36, pp.04202. ⟨10.1029/2008GL036206⟩
International audience; We report infrared spectrophotometric variability on the surface of Saturn's moon Titan detected in images returned by the Visual and Infrared Mapping Spectrometer (VIMS) onboard the Cassini Saturn Orbiter. The changes were ob
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::38d74dde33a1eb6f5a3fc4f48f48795a
https://ora.ox.ac.uk/objects/uuid:6ae22888-2b99-4a6f-99e0-0ee2bed83d1b
https://ora.ox.ac.uk/objects/uuid:6ae22888-2b99-4a6f-99e0-0ee2bed83d1b