Search

Your search keyword '"Sohl, F."' showing total 35 results
Start Over Author "Sohl, F." Topic enceladus
35 results on '"Sohl, F."'

2. TandEM: Titan and Enceladus mission

Author

Coustenis, A., Atreya, S. K., Balint, T., Brown, R. H., Dougherty, M. K., Ferri, F., Fulchignoni, M., Gautier, D., Gowen, R. A., Griffith, C. A., Gurvits, L. I., Jaumann, R., Langevin, Y., Leese, M. R., Lunine, J. I., McKay, C. P., Moussas, X., Müller-Wodarg, I., Neubauer, F., Owen, T. C., Raulin, F., Sittler, E. C., Sohl, F., Sotin, C., Tobie, G., Tokano, T., Turtle, E. P., Wahlund, J.-E., Waite, J. H., Baines, K. H., Blamont, J., Coates, A. J., Dandouras, I., Krimigis, T., Lellouch, E., Lorenz, R. D., Morse, A., Porco, C. C., Hirtzig, M., Saur, J., Spilker, T., Zarnecki, J. C., Choi, E., Achilleos, N., Amils, R., Annan, P., Atkinson, D. H., Bénilan, Y., Bertucci, C., Bézard, B., Bjoraker, G. L., Blanc, M., Boireau, L., Bouman, J., Cabane, M., Capria, M. T., Chassefière, E., Coll, P., Combes, M., Cooper, J. F., Coradini, A., Crary, F., Cravens, T., Daglis, I. A., de Angelis, E., de Bergh, C., de Pater, I., Dunford, C., Durry, G., Dutuit, O., Fairbrother, D., Flasar, F. M., Fortes, A. D., Frampton, R., Fujimoto, M., Galand, M., Grasset, O., Grott, M., Haltigin, T., Herique, A., Hersant, F., Hussmann, H., Ip, W., Johnson, R., Kallio, E., Kempf, S., Knapmeyer, M., Kofman, W., Koop, R., Kostiuk, T., Krupp, N., Küppers, M., Lammer, H., Lara, L.-M., Lavvas, P., Le Mouélic, S., Lebonnois, S., Ledvina, S., Li, J., Livengood, T. A., Lopes, R. M., Lopez-Moreno, J.-J., Luz, D., Mahaffy, P. R., Mall, U., Martinez-Frias, J., Marty, B., McCord, T., Menor Salvan, C., Milillo, A., Mitchell, D. G., Modolo, R., Mousis, O., Nakamura, M., Neish, C. D., Nixon, C. A., Nna Mvondo, D., Orton, G., Paetzold, M., Pitman, J., Pogrebenko, S., Pollard, W., Prieto-Ballesteros, O., Rannou, P., Reh, K., Richter, L., Robb, F. T., Rodrigo, R., Rodriguez, S., Romani, P., Ruiz Bermejo, M., Sarris, E. T., Schenk, P., Schmitt, B., Schmitz, N., Schulze-Makuch, D., Schwingenschuh, K., Selig, A., Sicardy, B., Soderblom, L., Spilker, L. J., Stam, D., Steele, A., Stephan, K., Strobel, D. F., Szego, K., Szopa, C., Thissen, R., Tomasko, M. G., Toublanc, D., Vali, H., Vardavas, I., Vuitton, V., West, R. A., Yelle, R., and Young, E. F.

Published
2009
Full Text
View/download PDF

3. Tidal dissipation in the ice-ocean system on Enceladus

Author

Hellard, H., Sohl, F., Van der Wal, W., Steinke, T., and Hussmann, H.

Subjects
internal ocean, tidal dissipation, Enceladus, composition, outer ice shell, Cassini-Huygens, interior structure
Published
2017

10. The exploration of habitable worlds with future space missions

Author

Coustenis, A., Encrenaz, T., Grasset, O., Solomonidou, A., Sohl, F., Hussmann, H., Wagner, F.W., Raulin, F, and Schulze-Makuch, D.

Subjects
tidal dissipation, Enceladus, habitability, solid body tides, JUpiter ICy moon Explorer (JUICE), Ganymede, future missions, Callisto, cryovolcanism, Europa, Titan, interior structure
Published
2013

11. Habitability potential of icy moons: a comparative study

Author

Coustenis, A., Solomonidou, A., Sohl, F., Bampasidis, G., Wagner, F.W., Raulin, F., and Schulze-Makuch, D.

Subjects
Enceladus, habitability, future missions, Ganymede, tides, outer solar system, Europa, Titan
Published
2013

32. ENCELADUS GEODETIC FRAMEWORK.

Author

Oberst, J., Hussmann, H., Giese, B., Sohl, F., Shoji, D., Stark, A., Wickhusen, K., and Wählisch, M.

Subjects
ENCELADUS (Satellite), SATURN (Planet)
Abstract

The small (approximately 500 km in diameter) satellite Enceladus is moving near the equatorial plane and deep in the gravity field of its parent planet Saturn. Owing to tidal interaction with its parent, Enceladus has adopted a pronounced 3-axial ellipsoidal shape and is tidally locked, with rotational and orbital periods of about 1.37 days. As the equator of Saturn is inclined to the planet's orbital plane, Enceladus, like most of the other satellites of Saturn, undergoes pronounced seasons. This paper gives a summary of the current status as well as shortcomings of our current knowledge regarding Enceladus' geodetic and dynamic parameters. [ABSTRACT FROM AUTHOR]

Published
2017
Full Text
View/download PDF

33. Degree-one convection and the origin of Enceladus' dichotomy

Author

Grott, M., Sohl, F., and Hussmann, H.

Subjects
*ENCELADUS (Satellite), *SOLAR system, *SATELLITES of Jupiter, *SATELLITES of Mars
Abstract

Abstract: Recently, the Cassini spacecraft has detected ongoing geologic activity near the south pole of Saturn''s moon Enceladus. In contrast, the satellite''s north-polar region is heavily cratered and appears to have been geologically inactive for a long time. We propose that this hemispheric dichotomy is caused by interior dynamics with degree-one convection driving the south-polar activity. We investigate a number of core sizes and internal heating rates for which degree-one convection occurs. The numerical simulations imply that a core radius of less than km and an energy input at a rate of 3.0 to 5.5 GW would be required for degree-one convection to prevail. This is within the range of the observed thermal power release near Enceladus'' south pole. Provided that Enceladus is not fully differentiated, degree-one convection is found to be a viable mechanism to explain Enceladus'' hemispheric dichotomy. [Copyright &y& Elsevier]

Published
2007
Full Text
View/download PDF

34. Non-steady state tidal heating of Enceladus.

Author

Shoji, D., Hussmann, H., Sohl, F., and Kurita, K.

Subjects
*STEADY state conduction, *TIDAL forces (Mechanics), *ENCELADUS (Satellite), *OCEAN surface topography, *HEAT pulses
Abstract

Highlights: [•] We analyze tidal heating of Enceladus coupling thermal and orbital states. [•] Episodic heat pulse is induced under some conditions. [•] Subsurface ocean appears cyclically, which may cause the localized ocean. [Copyright &y& Elsevier]

Published
2014
Full Text
View/download PDF

35. Ice rheology and tidal heating of Enceladus.

Author

Shoji, D., Hussmann, H., Kurita, K., and Sohl, F.

Subjects
*ICE crystals, *RHEOLOGY, *ENCELADUS (Satellite), *ANELASTICITY, *WASTE disposal in the ground, *MATHEMATICAL models
Abstract

Highlights: [•] Effect of anelasticity to Enceladus’ tidal heating is calculated. [•] In case of convective ice, less heat is generated than released at the surface. [•] For the Burgers model and conductive ice, a global subsurface water may be maintained. [Copyright &y& Elsevier]

Published
2013
Full Text
View/download PDF

Catalog

Books, media, physical & digital resources
See catalog results