Zobrazeno 1 - 10
of 1 853
pro vyhledávání: '"Vorburger, A."'
Autor:
Hamilton, Christopher W., McEwen, Alfred S., Keszthelyi, Laszlo, Carter, Lynn M., Davies, Ashley G., de Kleer, Katherine, Jessup, Kandis Lea, Jia, Xianzhe, Keane, James T., Mandt, Kathleen, Nimmo, Francis, Paranicas, Chris, Park, Ryan S., Perry, Jason E., Pommier, Anne, Radebaugh, Jani, Sutton, Sarah S., Vorburger, Audrey, Wurz, Peter, Borlina, Cauê, Haapala, Amanda F., DellaGiustina, Daniella N., Denevi, Brett W., Hörst, Sarah M., Kempf, Sascha, Khurana, Krishan K., Likar, Justin J., Masters, Adam, Mousis, Olivier, Polit, Anjani T., Bhushan, Aditya, Bland, Michael, Matsuyama, Isamu, Spencer, John
Jupiter's moon Io is a highly compelling target for future exploration that offers critical insight into tidal dissipation processes and the geology of high heat flux worlds, including primitive planetary bodies, such as the early Earth, that are sha
Externí odkaz:
http://arxiv.org/abs/2408.08334
Autor:
Roth, L., Blöcker, A., de Kleer, K., Goldstein, D., Lellouch, E., Saur, J., Schmidt, C., Strobel, D. F., Tao, C., Tsuchiya, F., Dols, V., Huybrighs, H., Mura, A., Szalay, J. R., Badman, S. V., de Pater, I., Dott, A. -C., Kagitani, M., Klaiber, L., Koga, R., McEwen, A., Milby, Z., Retherford, K. D., Schlegel, S., Thomas, N., Tseng, W. L., Vorburger, A.
Since the Voyager mission flybys in 1979, we have known the moon Io to be extremely volcanically active as well as to be the main source of plasma in the vast magnetosphere of Jupiter. Material lost from Io forms neutral clouds, the Io plasma torus a
Externí odkaz:
http://arxiv.org/abs/2403.13970
Autor:
Nittler, Larry R., Boujibar, Asmaa, Crapster-Pregont, Ellen, Frank, Elizabeth A., McCoy, Timothy J., McCubbin, Francis M., Starr, Richard D., Vorburger, Audrey, Weider, Shoshana Z.
Mercury, the innermost planet, formed under highly reduced conditions, based mainly on surface Fe, S, and Si abundances determined from MESSENGER mission data. The minor element Cr may serve as an independent oxybarometer, but only very limited Cr da
Externí odkaz:
http://arxiv.org/abs/2306.11859
So far no designated mission to either of the two ice giants, Uranus and Neptune, exists. Almost all of our gathered information on these planets comes from remote sensing. In recent years, NASA and ESA have started planning for future mission to Ura
Externí odkaz:
http://arxiv.org/abs/2306.09645
Electron impact ionization is critical in producing the ionospheres on many planetary bodies and, as discussed here, is critical for interpreting spacecraft and telescopic observations of the tenuous atmospheres of the icy Galilean satellites of Jupi
Externí odkaz:
http://arxiv.org/abs/2301.11380
Autor:
Mousis, O., Bouquet, A., Langevin, Y., André, N., Boithias, H., Durry, G., Faye, F., Hartogh, P., Helbert, J., Iess, L., Kempf, S., Masters, A., Postberg, F., Renard, J. -B., Vernazza, P., Vorburger, A., Wurz, P., Atkinson, D. H., Barabash, S., Berthomier, M., Brucato, J., Cable, M., Carter, J., Cazaux, S., Coustenis, A., Danger, G., Dehant, V., Fornaro, T., Garnier, P., Gautier, T., Groussin, O., Hadid, L. Z., Ize, J. -C., Kolmasova, I., Lebreton, J. -P., Maistre, S. Le, Lellouch, E., Lunine, J. I., Mandt, K. E., Martins, Z., Mimoun, D., Nenon, Q., Caro, G. M. Munõz, Rannou, P., Rauer, H., Schmitt-Kopplin, P., Schneeberger, A., Simons, M., Stephan, K., Van Hoolst, T., Vaverka, J., Wieser, M., Wörner, L.
Enceladus, an icy moon of Saturn, possesses an internal water ocean and jets expelling ocean material into space. Cassini investigations indicated that the subsurface ocean could be a habitable environment having a complex interaction with the rocky
Externí odkaz:
http://arxiv.org/abs/2211.00721
Autor:
Mogan, Shane R. Carberry, Tucker, Orenthal J., Johnson, Robert E., Roth, Lorenz, Alday, Juan, Vorburger, Audrey, Wurz, Peter, Galli, Andre, Smith, H. Todd, Marchand, Benoit, Oza, Apurva V.
We explore the parameter space for the contribution to Callisto's H corona observed by the Hubble Space Telescope (Roth et al. 2017a) from sublimated H2O and radiolytically produced H2 using the Direct Simulation Monte Carlo (DSMC) method. The spatia
Externí odkaz:
http://arxiv.org/abs/2210.14511
Autor:
Lammer, H., Scherf, M., Ito, Y., Mura, A., Vorburger, A., Guenther, E., Wurz, P., Erkaev, N. V., Odert, P.
In this review we discuss all the relevant solar/stellar radiation and plasma parameters and processes that act together in the formation and modification of atmospheres and exospheres that consist of surface-related minerals. Magma ocean degassed si
Externí odkaz:
http://arxiv.org/abs/2203.01656
Publikováno v:
In Current Opinion in Insect Science August 2024 64
Autor:
Jäggi, Noah, Gamborino, Diana, Bower, Dan J., Sossi, Paolo A., Wolf, Aaron S., Oza, Apurva V., Vorburger, Audrey, Galli, André, Wurz, Peter
Publikováno v:
Planet. Sci. J. 2 (2021) 230
MESSENGER observations suggest a magma ocean formed on proto-Mercury, during which evaporation of metals and outgassing of C- and H-bearing volatiles produced an early atmosphere. Atmospheric escape subsequently occurred by plasma heating, photoevapo
Externí odkaz:
http://arxiv.org/abs/2110.08093