Zobrazeno 1 - 10
of 174
pro vyhledávání: '"Cavalie, T"'
Autor:
Benne, B., Benmahi, B., Dobrijevic, M., Cavalié, T., Loison, J-C., Hickson, K. M., Barthélémy, M., Lilensten, J.
Publikováno v:
A&A, 686 (2024) A22
Due to its inclined orbit and the complex geometry of the magnetic field of Neptune, Triton experiences a highly variable magnetic environment. As precipitation of magnetospheric electrons is thought to have a large impact on the Triton atmosphere, a
Externí odkaz:
http://arxiv.org/abs/2407.16549
Autor:
Milcareck, G., Guerlet, S., Montmessin, F., Spiga, A., Leconte, J., Millour, E., Clément, N., Fletcher, L. N., Roman, M. T., Lellouch, E., Moreno, R., Cavalié, T., Carrión-González, Ó.
Publikováno v:
A&A 686, A303 (2024)
The observations made during the Voyager 2 flyby have shown that the stratosphere of Uranus and Neptune are warmer than expected by previous models. In addition, no seasonal variability of the thermal structure has been observed on Uranus since Voyag
Externí odkaz:
http://arxiv.org/abs/2403.13399
Publikováno v:
A&A 667, A169 (2022)
Triton is the largest satellite of Neptune and probably a Kuiper Belt Object that was captured by the planet. It has a tenuous nitrogen atmosphere similar to the one of Pluto and may be an ocean world. The Neptunian system has only been visited by Vo
Externí odkaz:
http://arxiv.org/abs/2209.04324
Autor:
Benmahi, B., Cavalié, T., Greathouse, T. K., Hue, V., Giles, R., Guerlet, S., Spiga, A., Cosentino, R.
Publikováno v:
A&A 652, A125 (2021)
Since the 1950s, quasi-periodic oscillations have been studied in the terrestrial equatorial stratosphere. Other planets of the solar system present (or are expected to present) such oscillations, like the Jupiter Equatorial Oscillation(JEO) and the
Externí odkaz:
http://arxiv.org/abs/2107.06122
Autor:
Cavalié, T., Benmahi, B., Hue, V., Moreno, R., Lellouch, E., Fouchet, T., Hartogh, P., Rezac, L., Greathouse, T. K., Gladstone, G. R., Sinclair, J. A., Dobrijevic, M., Billebaud, F., Jarchow, C.
Publikováno v:
Astronomy and Astrophysics, Volume 647, L8 (2021)
Context. The tropospheric wind pattern in Jupiter consists of alternating prograde and retrograde zonal jets with typical velocities of up to 100 m/s around the equator. At much higher altitudes, in the ionosphere, strong auroral jets have been disco
Externí odkaz:
http://arxiv.org/abs/2103.12208
Publikováno v:
Icarus 335 (2020), 113375
Neptune remains a mysterious world that deserves further exploration and is a high-priority objective for a future planetary mission in order to better understand the formation and evolution of ice giant planets. We have developed a coupled ion-neutr
Externí odkaz:
http://arxiv.org/abs/2011.07984
Autor:
Benmahi, B., Cavalié, T., Dobrijevic, M., Biver, N., Bermudez-Diaz, K., Sandqvist, Aa., Lellouch, E., Moreno, R., Fouchet, T., Hue, V., Hartogh, P., Billebaud, F., Lecacheux, A., Hjalmarson, Å., Frisk, U., Olberg, M., Team, andThe Odin
Publikováno v:
A&A 641, A140 (2020)
Comet Shoemaker-Levy 9 impacted Jupiter in July 1994, leaving its stratosphere with several new species, among them water vapor (H2O). With the aid of a photochemical model H2O can be used as a dynamical tracer in the jovian stratosphere. In this pap
Externí odkaz:
http://arxiv.org/abs/2007.05415
Comparatively little is known about atmospheric chemistry on Uranus and Neptune, because remote spectral observations of these cold, distant ``Ice Giants'' are challenging, and each planet has only been visited by a single spacecraft during brief fly
Externí odkaz:
http://arxiv.org/abs/2006.11367
Autor:
Mousis, O., Aguichine, A., Atkinson, D. H., Atreya, S. K., Cavalié, T., Lunine, J. I., Mandt, K. E., Ronnet, T.
We investigate the enrichment patterns of several delivery scenarios of the volatiles to the atmospheres of ice giants, having in mind that the only well constrained determination made remotely, i.e. the carbon abundance measurement, suggests that th
Externí odkaz:
http://arxiv.org/abs/2004.11061
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.