Zobrazeno 1 - 10
of 133
pro vyhledávání: '"S M, Wahl"'
We study the response of hot Jupiters to a static tidal perturbation using the concentric MacLaurin spheroid method. For strongly irradiated planets, we first performed radiative transfer calculations to relate the planet's equilibrium temperature, T
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::06840e04c3c46d68ad61682992b84989
https://resolver.caltech.edu/CaltechAUTHORS:20211116-182110554
https://resolver.caltech.edu/CaltechAUTHORS:20211116-182110554
Since its arrival at Jupiter in 2016, the Juno spacecraft has measured the planet’s gravity fields with unprecedented precision. The interpretation of these measurements has been challenging because the magnitudes of the gravity coefficients J4 and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fb276779ddf2ff36973188a86b20491e
https://doi.org/10.5194/egusphere-egu21-9083
https://doi.org/10.5194/egusphere-egu21-9083
Autor:
Ravit Helled, S. M. Wahl, Steven Levin, Luciano Iess, Jonathan I. Lunine, Scott Bolton, William B. Hubbard, D. J. Stevenson, Daniel R. Reese, Daniele Durante, Tristan Guillot, Eli Galanti, Hao Cao, Yamila Miguel, Marzia Parisi, W. M. Folkner, Yohai Kaspi, John E. P. Connerney, A. Biekman, Burkhard Militzer
Publikováno v:
Nature
Nature, Nature Publishing Group, 2018, 555 (7695), pp.227-230. ⟨10.1038/nature25775⟩
Nature, 2018, 555 (7695), pp.227-230. ⟨10.1038/nature25775⟩
Nature, 555, 227-230
Nature, Nature Publishing Group, 2018, 555 (7695), pp.227-230. ⟨10.1038/nature25775⟩
Nature, 2018, 555 (7695), pp.227-230. ⟨10.1038/nature25775⟩
Nature, 555, 227-230
International audience; Jupiter’s atmosphere is rotating differentially, with zones and belts rotating at speeds that differ by up to 100 metres per second. Whether this is also true of the gas giant’s interior has been unknown1,2, limiting our a
Autor:
Steven Levin, Yohai Kaspi, Scott Bolton, Burkhard Militzer, Ravit Helled, Yamila Miguel, William B. Hubbard, John E. P. Connerney, S. M. Wahl, Eli Galanti, Tristan Guillot
Publikováno v:
Geophysical Research Letters. 44:5960-5968
Israeli Ministry of Science; Minerva foundation; Federal German Ministry of Education and Research; Helen Kimmel Center for Planetary Science at the Weizmann Institute of Science; CNES; BSF; NSF; Juno project
The Cassini spacecraft's Grand Finale orbits provided a unique opportunity to probe Saturn's gravity field and interior structure. Doppler measurements yielded unexpectedly large values for the gravity harmonics J_6, J_8, and J_10 that cannot be matc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::04615b8c66bb94030b808f871e49b63d
http://arxiv.org/abs/1905.08907
http://arxiv.org/abs/1905.08907
Autor:
Luciano Iess, Marco Zannoni, Paolo Tortora, P. Racioppa, Burkhard Militzer, A. Anabtawi, Daniele Durante, Eli Galanti, William B. Hubbard, Yohai Kaspi, S. M. Wahl, Mirco Junior Mariani, P. D. Nicholson
Cassini's last look at Saturn's rings During the final stages of the Cassini mission, the spacecraft flew between the planet and its rings, providing a new view on this spectacular system (see the Perspective by Ida). Setting the scene, Spilker revie
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f7c1ed9589643b7d3f9a9026b2b0efd9
http://hdl.handle.net/11573/1402780
http://hdl.handle.net/11573/1402780
Publikováno v:
Journal of Geophysical Research: Planets. 121:1552-1572
This article provides an overview of how models of giant planet interiors are constructed. We review measurements from past space missions that provide constraints for the interior structure of Jupiter. We discuss typical three-layer interior models
Publikováno v:
The Astrophysical Journal. 891:42
Autor:
Burkhard Militzer, John E. P. Connerney, William B. Hubbard, Jeremy Bloxham, Marzia Parisi, Ravit Helled, Luciano Iess, Tristan Guillot, Andrew P. Ingersoll, Daniele Durante, Eli Galanti, Steven Levin, Scott Bolton, Jonathan I. Lunine, Yamila Miguel, D. J. Stevenson, Hao Cao, Yohai Kaspi, S. M. Wahl, William M. Folkner
Publikováno v:
Nature
Nature, Nature Publishing Group, 2018, 555 (7695), pp.223-226. ⟨10.1038/nature25793⟩
Nature, 555, 223-226
Nature, Nature Publishing Group, 2018, 555 (7695), pp.223-226. ⟨10.1038/nature25793⟩
Nature, 555, 223-226
The depth to which Jupiter’s observed east–west jet streams extend has been a long-standing question. Resolving this puzzle has been a primary goal for the Juno spacecraft, which has been in orbit around the gas giant since July 2016. Juno’s gr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c49f480b87acf6da28e3abfc242c6453
https://hal.archives-ouvertes.fr/hal-02307984
https://hal.archives-ouvertes.fr/hal-02307984
Autor:
S. M. Wahl, Jonathan I. Lunine, L. Gomez Casajus, Burkhard Militzer, Ryan S. Park, Andrea Milani, Dustin Buccino, William B. Hubbard, Paolo Tortora, Luciano Iess, Steven Levin, Marzia Parisi, Ravit Helled, Daniele Durante, Eli Galanti, Yamila Miguel, W. M. Folkner, Marco Zannoni, Scott Bolton, John D. Anderson, Daniele Serra, D. J. Stevenson, P. Racioppa, Tristan Guillot, Yohai Kaspi, Hao Cao, John E. P. Connerney
Publikováno v:
Nature
Nature, Nature Publishing Group, 2018, 555 (7695), pp.220-222. ⟨10.1038/nature25776⟩
Nature, Nature Publishing Group, 2018, 555 (7695), pp.220-222. ⟨10.1038/nature25776⟩
The gravity harmonics of a fluid, rotating planet can be decomposed into static components arising from solid-body rotation and dynamic components arising from flows. In the absence of internal dynamics, the gravity field is axially and hemispherical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0526681ebda67ed530b877795e0c8947
https://hal.univ-cotedazur.fr/hal-02528883
https://hal.univ-cotedazur.fr/hal-02528883