Spectral properties of icy saturnian satellites derived from cassini data

K. Stephan; R. Jaumann; R. Wagner; R. N. Clark; D. P. Cruikshank; C. Dalle Ore; R. H. Brown; B. Giese; T. Roatsch; D. Matson; K. Baines; G. Filiacchione; F. Cappacione; B. J. Buratti; P. D. Nicholson

doi:10.1109/WHISPERS.2014.8077516

Spectral properties of icy saturnian satellites derived from cassini data

K. Stephan, R. Jaumann, R. Wagner, R. N. Clark, D. P. Cruikshank, C. Dalle Ore, R. H. Brown, B. Giese, T. Roatsch, D. Matson, K. Baines, G. Filiacchione, F. Cappacione, B. J. Buratti, P. D. Nicholson

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

Cassini's Visual and Infrared Mapping Spectrometer (VIMS) offers the first spatially resolved hyperspectral data of the Saturnian satellites [1] allowing a detailed comparison of their spectral properties including their spatial distribution across the satellite's surface. Additionally, images acquired by the Cassini ISS cameras [2] offer the opportunity to study any relationships between the spectral variations to geological and morphological surface features. This is essential to understand the origin of the major and especially minor surface compounds and/or their physical properties. Either, the derived spectral variations are closely related to the surface geology of the specific satellite, or they can be explained by the interaction of the surface material and the space environment (including the planets magnetosphere). Thus, the analysis of the icy satellites spectral properties not only further our understanding of the icy satellites evolution but also complete our view about the whole planetary system.

Original language	English (US)
Title of host publication	2014 6th Workshop on Hyperspectral Image and Signal Processing
Subtitle of host publication	Evolution in Remote Sensing, WHISPERS 2014
Publisher	IEEE Computer Society
ISBN (Electronic)	9781467390125
DOIs	https://doi.org/10.1109/WHISPERS.2014.8077516
State	Published - Oct 19 2017
Externally published	Yes
Event	6th Workshop on Hyperspectral Image and Signal Processing: Evolution in Remote Sensing, WHISPERS 2014 - Lausanne, Switzerland Duration: Jun 24 2014 → Jun 27 2014

Publication series

Name	Workshop on Hyperspectral Image and Signal Processing, Evolution in Remote Sensing
Volume	2014-June
ISSN (Print)	2158-6276

Other

Other	6th Workshop on Hyperspectral Image and Signal Processing: Evolution in Remote Sensing, WHISPERS 2014
Country/Territory	Switzerland
City	Lausanne
Period	6/24/14 → 6/27/14

Keywords

Cassini mission
Saturnian satellites
icy geology
spectroscopy
surface composition

ASJC Scopus subject areas

Computer Vision and Pattern Recognition
Signal Processing

Access to Document

10.1109/WHISPERS.2014.8077516

Cite this

Stephan, K., Jaumann, R., Wagner, R., Clark, R. N., Cruikshank, D. P., Dalle Ore, C., Brown, R. H., Giese, B., Roatsch, T., Matson, D., Baines, K., Filiacchione, G., Cappacione, F., Buratti, B. J., & Nicholson, P. D. (2017). Spectral properties of icy saturnian satellites derived from cassini data. In 2014 6th Workshop on Hyperspectral Image and Signal Processing: Evolution in Remote Sensing, WHISPERS 2014 [8077516] (Workshop on Hyperspectral Image and Signal Processing, Evolution in Remote Sensing; Vol. 2014-June). IEEE Computer Society. https://doi.org/10.1109/WHISPERS.2014.8077516

Spectral properties of icy saturnian satellites derived from cassini data. / Stephan, K.; Jaumann, R.; Wagner, R.; Clark, R. N.; Cruikshank, D. P.; Dalle Ore, C.; Brown, R. H.; Giese, B.; Roatsch, T.; Matson, D.; Baines, K.; Filiacchione, G.; Cappacione, F.; Buratti, B. J.; Nicholson, P. D.

2014 6th Workshop on Hyperspectral Image and Signal Processing: Evolution in Remote Sensing, WHISPERS 2014. IEEE Computer Society, 2017. 8077516 (Workshop on Hyperspectral Image and Signal Processing, Evolution in Remote Sensing; Vol. 2014-June).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Stephan, K, Jaumann, R, Wagner, R, Clark, RN, Cruikshank, DP, Dalle Ore, C, Brown, RH, Giese, B, Roatsch, T, Matson, D, Baines, K, Filiacchione, G, Cappacione, F, Buratti, BJ & Nicholson, PD 2017, Spectral properties of icy saturnian satellites derived from cassini data. in 2014 6th Workshop on Hyperspectral Image and Signal Processing: Evolution in Remote Sensing, WHISPERS 2014., 8077516, Workshop on Hyperspectral Image and Signal Processing, Evolution in Remote Sensing, vol. 2014-June, IEEE Computer Society, 6th Workshop on Hyperspectral Image and Signal Processing: Evolution in Remote Sensing, WHISPERS 2014, Lausanne, Switzerland, 6/24/14. https://doi.org/10.1109/WHISPERS.2014.8077516

Stephan K, Jaumann R, Wagner R, Clark RN, Cruikshank DP, Dalle Ore C et al. Spectral properties of icy saturnian satellites derived from cassini data. In 2014 6th Workshop on Hyperspectral Image and Signal Processing: Evolution in Remote Sensing, WHISPERS 2014. IEEE Computer Society. 2017. 8077516. (Workshop on Hyperspectral Image and Signal Processing, Evolution in Remote Sensing). https://doi.org/10.1109/WHISPERS.2014.8077516

Stephan, K. ; Jaumann, R. ; Wagner, R. ; Clark, R. N. ; Cruikshank, D. P. ; Dalle Ore, C. ; Brown, R. H. ; Giese, B. ; Roatsch, T. ; Matson, D. ; Baines, K. ; Filiacchione, G. ; Cappacione, F. ; Buratti, B. J. ; Nicholson, P. D. / Spectral properties of icy saturnian satellites derived from cassini data. 2014 6th Workshop on Hyperspectral Image and Signal Processing: Evolution in Remote Sensing, WHISPERS 2014. IEEE Computer Society, 2017. (Workshop on Hyperspectral Image and Signal Processing, Evolution in Remote Sensing).

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abstract = "Cassini's Visual and Infrared Mapping Spectrometer (VIMS) offers the first spatially resolved hyperspectral data of the Saturnian satellites [1] allowing a detailed comparison of their spectral properties including their spatial distribution across the satellite's surface. Additionally, images acquired by the Cassini ISS cameras [2] offer the opportunity to study any relationships between the spectral variations to geological and morphological surface features. This is essential to understand the origin of the major and especially minor surface compounds and/or their physical properties. Either, the derived spectral variations are closely related to the surface geology of the specific satellite, or they can be explained by the interaction of the surface material and the space environment (including the planets magnetosphere). Thus, the analysis of the icy satellites spectral properties not only further our understanding of the icy satellites evolution but also complete our view about the whole planetary system.",

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author = "K. Stephan and R. Jaumann and R. Wagner and Clark, {R. N.} and Cruikshank, {D. P.} and {Dalle Ore}, C. and Brown, {R. H.} and B. Giese and T. Roatsch and D. Matson and K. Baines and G. Filiacchione and F. Cappacione and Buratti, {B. J.} and Nicholson, {P. D.}",

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AU - Dalle Ore, C.

AU - Brown, R. H.

AU - Giese, B.

AU - Roatsch, T.

AU - Matson, D.

AU - Baines, K.

AU - Filiacchione, G.

AU - Cappacione, F.

AU - Buratti, B. J.

AU - Nicholson, P. D.

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N2 - Cassini's Visual and Infrared Mapping Spectrometer (VIMS) offers the first spatially resolved hyperspectral data of the Saturnian satellites [1] allowing a detailed comparison of their spectral properties including their spatial distribution across the satellite's surface. Additionally, images acquired by the Cassini ISS cameras [2] offer the opportunity to study any relationships between the spectral variations to geological and morphological surface features. This is essential to understand the origin of the major and especially minor surface compounds and/or their physical properties. Either, the derived spectral variations are closely related to the surface geology of the specific satellite, or they can be explained by the interaction of the surface material and the space environment (including the planets magnetosphere). Thus, the analysis of the icy satellites spectral properties not only further our understanding of the icy satellites evolution but also complete our view about the whole planetary system.

AB - Cassini's Visual and Infrared Mapping Spectrometer (VIMS) offers the first spatially resolved hyperspectral data of the Saturnian satellites [1] allowing a detailed comparison of their spectral properties including their spatial distribution across the satellite's surface. Additionally, images acquired by the Cassini ISS cameras [2] offer the opportunity to study any relationships between the spectral variations to geological and morphological surface features. This is essential to understand the origin of the major and especially minor surface compounds and/or their physical properties. Either, the derived spectral variations are closely related to the surface geology of the specific satellite, or they can be explained by the interaction of the surface material and the space environment (including the planets magnetosphere). Thus, the analysis of the icy satellites spectral properties not only further our understanding of the icy satellites evolution but also complete our view about the whole planetary system.

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Spectral properties of icy saturnian satellites derived from cassini data

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