Touring the saturnian system: the atmospheres of titan and saturn
Abstract This report follows the presentation originally given in the ESA Phase A Study for the Cassini Huygens Mission. The combination of the Huygens atmospheric probe into Titan's atmosphere with the Cassini orbiter allows for both in-situ and remote-sensing observations of Titan. This not o...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Owen, Tobias [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2002 |
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| Schlagwörter: |
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| Anmerkung: |
© Kluwer Academic Publishers 2002 |
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| Übergeordnetes Werk: |
Enthalten in: Space science reviews - Kluwer Academic Publishers, 1962, 104(2002), 1-4 vom: Juli, Seite 347-376 |
|---|---|
| Übergeordnetes Werk: |
volume:104 ; year:2002 ; number:1-4 ; month:07 ; pages:347-376 |
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|---|
| DOI / URN: |
10.1023/A:1023684406168 |
|---|
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OLC2033687309 |
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10.1023/A:1023684406168 doi (DE-627)OLC2033687309 (DE-He213)A:1023684406168-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Owen, Tobias verfasserin aut Touring the saturnian system: the atmospheres of titan and saturn 2002 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2002 Abstract This report follows the presentation originally given in the ESA Phase A Study for the Cassini Huygens Mission. The combination of the Huygens atmospheric probe into Titan's atmosphere with the Cassini orbiter allows for both in-situ and remote-sensing observations of Titan. This not only provides a rich harvest of data about Saturn's famous satellite but will permit a useful calibration of the remote-sensing instruments which will also be used on Saturn itself. Composition, thermal structure, dynamics, aeronomy, magnetosphere interactions and origins will all be investigated for the two atmospheres, and the spacecraft will also deliver information on the interiors of both Titan and Saturn. As the surface of Titan is intimately linked with the atmosphere, we also discuss some of the surface studies that will be carried out by both probe and orbiter. Zonal Wind Giant Planet Radio Occultation Solar Nebula Radio Occultation Measurement Gautier, Daniel aut Enthalten in Space science reviews Kluwer Academic Publishers, 1962 104(2002), 1-4 vom: Juli, Seite 347-376 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:104 year:2002 number:1-4 month:07 pages:347-376 https://doi.org/10.1023/A:1023684406168 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 104 2002 1-4 07 347-376 |
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10.1023/A:1023684406168 doi (DE-627)OLC2033687309 (DE-He213)A:1023684406168-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Owen, Tobias verfasserin aut Touring the saturnian system: the atmospheres of titan and saturn 2002 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2002 Abstract This report follows the presentation originally given in the ESA Phase A Study for the Cassini Huygens Mission. The combination of the Huygens atmospheric probe into Titan's atmosphere with the Cassini orbiter allows for both in-situ and remote-sensing observations of Titan. This not only provides a rich harvest of data about Saturn's famous satellite but will permit a useful calibration of the remote-sensing instruments which will also be used on Saturn itself. Composition, thermal structure, dynamics, aeronomy, magnetosphere interactions and origins will all be investigated for the two atmospheres, and the spacecraft will also deliver information on the interiors of both Titan and Saturn. As the surface of Titan is intimately linked with the atmosphere, we also discuss some of the surface studies that will be carried out by both probe and orbiter. Zonal Wind Giant Planet Radio Occultation Solar Nebula Radio Occultation Measurement Gautier, Daniel aut Enthalten in Space science reviews Kluwer Academic Publishers, 1962 104(2002), 1-4 vom: Juli, Seite 347-376 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:104 year:2002 number:1-4 month:07 pages:347-376 https://doi.org/10.1023/A:1023684406168 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 104 2002 1-4 07 347-376 |
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10.1023/A:1023684406168 doi (DE-627)OLC2033687309 (DE-He213)A:1023684406168-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Owen, Tobias verfasserin aut Touring the saturnian system: the atmospheres of titan and saturn 2002 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2002 Abstract This report follows the presentation originally given in the ESA Phase A Study for the Cassini Huygens Mission. The combination of the Huygens atmospheric probe into Titan's atmosphere with the Cassini orbiter allows for both in-situ and remote-sensing observations of Titan. This not only provides a rich harvest of data about Saturn's famous satellite but will permit a useful calibration of the remote-sensing instruments which will also be used on Saturn itself. Composition, thermal structure, dynamics, aeronomy, magnetosphere interactions and origins will all be investigated for the two atmospheres, and the spacecraft will also deliver information on the interiors of both Titan and Saturn. As the surface of Titan is intimately linked with the atmosphere, we also discuss some of the surface studies that will be carried out by both probe and orbiter. Zonal Wind Giant Planet Radio Occultation Solar Nebula Radio Occultation Measurement Gautier, Daniel aut Enthalten in Space science reviews Kluwer Academic Publishers, 1962 104(2002), 1-4 vom: Juli, Seite 347-376 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:104 year:2002 number:1-4 month:07 pages:347-376 https://doi.org/10.1023/A:1023684406168 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 104 2002 1-4 07 347-376 |
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10.1023/A:1023684406168 doi (DE-627)OLC2033687309 (DE-He213)A:1023684406168-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Owen, Tobias verfasserin aut Touring the saturnian system: the atmospheres of titan and saturn 2002 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2002 Abstract This report follows the presentation originally given in the ESA Phase A Study for the Cassini Huygens Mission. The combination of the Huygens atmospheric probe into Titan's atmosphere with the Cassini orbiter allows for both in-situ and remote-sensing observations of Titan. This not only provides a rich harvest of data about Saturn's famous satellite but will permit a useful calibration of the remote-sensing instruments which will also be used on Saturn itself. Composition, thermal structure, dynamics, aeronomy, magnetosphere interactions and origins will all be investigated for the two atmospheres, and the spacecraft will also deliver information on the interiors of both Titan and Saturn. As the surface of Titan is intimately linked with the atmosphere, we also discuss some of the surface studies that will be carried out by both probe and orbiter. Zonal Wind Giant Planet Radio Occultation Solar Nebula Radio Occultation Measurement Gautier, Daniel aut Enthalten in Space science reviews Kluwer Academic Publishers, 1962 104(2002), 1-4 vom: Juli, Seite 347-376 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:104 year:2002 number:1-4 month:07 pages:347-376 https://doi.org/10.1023/A:1023684406168 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 104 2002 1-4 07 347-376 |
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Abstract This report follows the presentation originally given in the ESA Phase A Study for the Cassini Huygens Mission. The combination of the Huygens atmospheric probe into Titan's atmosphere with the Cassini orbiter allows for both in-situ and remote-sensing observations of Titan. This not only provides a rich harvest of data about Saturn's famous satellite but will permit a useful calibration of the remote-sensing instruments which will also be used on Saturn itself. Composition, thermal structure, dynamics, aeronomy, magnetosphere interactions and origins will all be investigated for the two atmospheres, and the spacecraft will also deliver information on the interiors of both Titan and Saturn. As the surface of Titan is intimately linked with the atmosphere, we also discuss some of the surface studies that will be carried out by both probe and orbiter. © Kluwer Academic Publishers 2002 |
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Abstract This report follows the presentation originally given in the ESA Phase A Study for the Cassini Huygens Mission. The combination of the Huygens atmospheric probe into Titan's atmosphere with the Cassini orbiter allows for both in-situ and remote-sensing observations of Titan. This not only provides a rich harvest of data about Saturn's famous satellite but will permit a useful calibration of the remote-sensing instruments which will also be used on Saturn itself. Composition, thermal structure, dynamics, aeronomy, magnetosphere interactions and origins will all be investigated for the two atmospheres, and the spacecraft will also deliver information on the interiors of both Titan and Saturn. As the surface of Titan is intimately linked with the atmosphere, we also discuss some of the surface studies that will be carried out by both probe and orbiter. © Kluwer Academic Publishers 2002 |
| abstract_unstemmed |
Abstract This report follows the presentation originally given in the ESA Phase A Study for the Cassini Huygens Mission. The combination of the Huygens atmospheric probe into Titan's atmosphere with the Cassini orbiter allows for both in-situ and remote-sensing observations of Titan. This not only provides a rich harvest of data about Saturn's famous satellite but will permit a useful calibration of the remote-sensing instruments which will also be used on Saturn itself. Composition, thermal structure, dynamics, aeronomy, magnetosphere interactions and origins will all be investigated for the two atmospheres, and the spacecraft will also deliver information on the interiors of both Titan and Saturn. As the surface of Titan is intimately linked with the atmosphere, we also discuss some of the surface studies that will be carried out by both probe and orbiter. © Kluwer Academic Publishers 2002 |
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Touring the saturnian system: the atmospheres of titan and saturn |
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