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pro vyhledávání: '"Reh, K. R."'
Autor:
Mousis, O., Fletcher, L. N., Lebreton, J. -P., Wurz, P., Cavalié, T., Coustenis, A., Courtin, R., Gautier, D., Helled, R., Irwin, P. G. J., Morse, A. D., Nettelmann, N., Marty, B., Rousselot, P., Venot, O., Atkinson, D. H., Waite, J. H., Reh, K. R., Simon-Miller, A., Atreya, S., André, N., Blanc, M., Daglis, I. A., Fischer, G., Geppert, W. D., Guillot, T., Hedman, M. M., Hueso, R., Lellouch, E., Lunine, J. I., Murray, C. D., O'Donoghue, J., Rengel, M., Sanchez-Lavega, A., Schmider, F. -X., Spiga, A., Spilker, T., Petit, J. -M., Tiscareno, M. S., Ali-Dib, M., Altwegg, K., Bouquet, A., Briois, C., Fouchet, T., Guerlet, S., Kostiuk, T., Lebleu, D., Moreno, R., Orton, G. S., Poncy, J.
Remote sensing observations meet some limitations when used to study the bulk atmospheric composition of the giant planets of our solar system. A remarkable example of the superiority of in situ probe measurements is illustrated by the exploration of
Externí odkaz:
http://arxiv.org/abs/1404.4811
Autor:
Mitri, G., Postberg, F., Soderblom, J. M., Tobie, G., Tortora, P., Wurz, P., Barnes, J. W., Carrasco, N., Coustenis, A., Ferri, F., Hayes, A., Hillier, J., Kempf, S., Lebreton, J. P., Lorenz, R. D., OROSEI, ROBERTO, Petropoulos, A. E. E., Reh, K. R., Schmidt, J., Sotin, C., Srama, R., Vuitton, V., Yen, C. W.
The NASA-ESA-ASI Cassini-Huygens mission has revealed Titan and Enceladus to be two of the most enigmatic worlds in the Solar System. Titan, with its organically rich and dynamic atmosphere and geology, and Enceladus, with its active plume of water v
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______4759::d7dff670e03a527959c51f1292a95f77
http://hdl.handle.net/20.500.12386/26040
http://hdl.handle.net/20.500.12386/26040
Autor:
Mousis, O., Fletcher, L. N., Lebreton, J.-P., Wurz, P., Cavalié, T., Coustenis, A., Atkinson, D. H., Atreya, S., Gautier, D., Guillot, T., Lunine, J. I., Marty, B., Morse, A. D., Reh, K. R., Simon-Miller, A., Spilker, T., Waite, J. H.
Publikováno v:
Planetary Space Science
45th Lunar and Planetary Science Conference
45th Lunar and Planetary Science Conference
Remote sensing observations meet some limitations when used to study the bulk atmospheric composition of the giant planets of our solar system. A remarkable example of the superiority of in situ probe measurements is illustrated by the exploration of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c809b6dd63b78069afffab3add39d64f
http://www.hou.usra.edu/meetings/lpsc2014/pdf/1261.pdf
http://www.hou.usra.edu/meetings/lpsc2014/pdf/1261.pdf
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