Zobrazeno 1 - 10
of 46
pro vyhledávání: '"S. K. ATREYA"'
Autor:
Y. Miguel, M. Bazot, T. Guillot, S. Howard, E. Galanti, Y. Kaspi, W. B. Hubbard, B. Militzer, R. Helled, S. K. Atreya, J. E. P. Connerney, D. Durante, L. Kulowski, J. I. Lunine, D. Stevenson, S. Bolton
Publikováno v:
Astronomy & Astrophysics, 662:A18
While Jupiter's massive gas envelope consists mainly of hydrogen and helium, the key to understanding Jupiter's formation and evolution lies in the distribution of the remaining (heavy) elements. Before the Juno mission, the lack of high-precision gr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c6ac3d4235c023a08f7a0348e4e24a8c
http://arxiv.org/abs/2203.01866
http://arxiv.org/abs/2203.01866
Autor:
Zhimeng Zhang, Heidi N. Becker, Yohai Kaspi, Cheng Li, Paul G. Steffes, Leigh N. Fletcher, Fabiano Oyafuso, Tristan Guillot, Scott Bolton, Rakesh K. Yadav, Andrew P. Ingersoll, J. Lunine, Sidharth Misra, Eli Galanti, Steve Levin, S. K. Atreya, Michael H. Wong, Samuel Gulkis, David J. Stevenson, M. Allison, Shannon Brown, J. K. Arballo, Jeremy Bloxham, M. A. Janssen, J. H. Waite, G. S. Orton
Publikováno v:
Science
Measuring the depth of Jupiter’s storms The atmosphere of Jupiter consists of bands of winds rotating at different rates, punctuated by giant storms. The largest storm is the Great Red Spot (GRS), which has persisted for more than a century. It has
Autor:
Francesca Altieri, Christina Plainaki, Alessandra Migliorini, John E. P. Connerney, Scott Bolton, Jean-Claude Gérard, A. Olivieri, Bianca Maria Dinelli, S. K. Atreya, Alessandro Mura, M. L. Moriconi, Alberto Adriani, G. Piccioni, Andrea Cicchetti, Raffaella Noschese, Steve Levin, Davide Grassi, Giuseppe Sindoni, Roberto Sordini, Federico Tosi
Publikováno v:
Icarus. 329:132-139
NASA's Juno spacecraft has been orbiting Jupiter since August 2016, providing unprecedented insights into the giant planet's atmosphere. The Jupiter Infrared Auroral Mapper (JIRAM) experiment on board Juno has made spectroscopic observations of the t
Autor:
Roberto Sordini, Stefania Stefani, Giuseppe Sindoni, Scott Bolton, S. K. Atreya, Bianca Maria Dinelli, Alberto Adriani, Andrea Cicchetti, Raffaella Noschese, Christina Plainaki, Alessandra Migliorini, Jonathan I. Lunine, Federico Tosi, Davide Grassi, Diego Turrini, Alessandro Mura, Leigh N. Fletcher, Francesca Altieri, G. Piccioni, Glenn S. Orton, Maria Luisa Moriconi, A. Olivieri, Gianrico Filacchione
Publikováno v:
Journal of Geophysical Research: Planets
The spatial distribution of water, ammonia, phosphine, germane, and arsine in the Jupiter's troposphere has been inferred from the Jovian Infrared Auroral Mapper (JIRAM) Juno data. Measurements allow us to retrieve the vertically averaged concentrati
Publikováno v:
Astronomy & Astrophysics
Autor:
Glenn S. Orton, Fran Bagenal, Alberto Adriani, Andrea Cicchetti, Steven Levin, A. Olivieri, Federico Tosi, Candice Hansen, Marilena Amoroso, Raffaella Noschese, Diego Turrini, Gianrico Filacchione, Giuseppe Sindoni, Bianca Maria Dinelli, F. Fabiano, Jonathan I. Lunine, Maria Luisa Moriconi, Francesca Altieri, Giuseppe Piccioni, Stefania Stefani, S. K. Atreya, Andrew P. Ingersoll, John E. P. Connerney, Davide Grassi, Scott Bolton, M. A. Janssen, Alessandra Migliorini, Alessandro Mura
Publikováno v:
Geophysical Research Letters. 44:4660-4668
During the first perijove passage of the Juno mission, the Jovian InfraRed Auroral Mapper (JIRAM) observed a line of closely spaced oval features in Jupiter's southern hemisphere, between 30°S and 45°S. In this work, we focused on the longitudinal
Autor:
Matthew J. Richter, Frank Daerden, L. Neary, Marco Giuranna, T. Fouchet, Shohei Aoki, T. Encrenaz, S. K. Atreya, B. Bézard, Frank Montmessin, Thomas K. Greathouse, François Forget, Sébastien Viscardy, Curtis DeWitt, Franck Lefèvre
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 627, A 60 (10p.). ⟨10.1051/0004-6361/201935300⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 627, A 60 (10p.). ⟨10.1051/0004-6361/201935300⟩
We pursued our ground-based seasonal monitoring of hydrogen peroxide on Mars using thermal imaging spectroscopy, with two observations of the planet near opposition, in May 2016 (solar longitude Ls = 148.5°, diameter = 17 arcsec) and July 2018 (Ls =
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7042b9497dc5bbd1dd1eda6d65e3249f
https://hal-insu.archives-ouvertes.fr/insu-02151733/document
https://hal-insu.archives-ouvertes.fr/insu-02151733/document
Autor:
A. Adriani, A. Mura, M. L. Moriconi, B. M. Dinelli, F. Fabiano, F. Altieri, G. Sindoni, S. J. Bolton, J. E. P. Connerney, S. K. Atreya, F. Bagenal, J. -C. M. C. G\'erard, G. Filacchione, F. Tosi, A. Migliorini, D. Grassi, G. Piccioni, R. Noschese, A. Cicchetti, G. R. Gladstone, C. Hansen, W. S. Kurth, S. M. Levin, B. H. Mauk, D. J. McComas, A. Olivieri, D. Turrini, S. Stefani, M. Amoroso
The Jupiter InfraRed Auroral Mapper (JIRAM) aboard Juno observed the Jovian South Pole aurora during the first orbit of the mission. H 3+ (trihydrogen cation) and CH 4 (methane) emissions have been identified and measured. The observations have been
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______4094::d1dba7a037b9d4848b9ab083707fd89e
http://hdl.handle.net/11585/630573
http://hdl.handle.net/11585/630573
Autor:
M. L. Moriconi, A. Adriani, B. M. Dinelli, F. Fabiano, F. Altieri, F. Tosi, G. Filacchione, A. Migliorini, J. C. G'erard, A. Mura, D. Grassi, G. Sindoni, G. Piccioni, R. Noschese, A. Cicchetti, S. J. Bolton, J. E. P. Connerney, S. K. Atreya, F. Bagenal, G. R. Gladstone, C. Hansen, W. S. Kurth, S. M. Levin, B. H. Mauk, D. J. McComas, D. Turrini, S. Stefani, A. Olivieri, M. Amoroso
Throughout the first orbit of the NASA Juno mission around Jupiter, the Jupiter InfraRed Auroral Mapper (JIRAM) targeted the northern and southern polar regions several times. The analyses of the acquired images and spectra confirmed a significant pr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::277dc693bad669292e0eff139000466d
http://hdl.handle.net/20.500.12386/30589
http://hdl.handle.net/20.500.12386/30589
Autor:
B. M. Dinelli, F. Fabiano, A. Adriani, F. Altieri, M. L. Moriconi, A. Mura, G. Sindoni, G. Filacchione, F. Tosi, A. Migliorini, D. Grassi, G. Piccioni, R. Noschese, A. Cicchetti, S. J. Bolton, J. E. P. Connerney, S. K. Atreya, F. Bagenal, G. R. Gladstone, C. J. Hansen, W. S. Kurth, S. M. Levin, B. H. Mauk, D. J. McComas, J. -C. G`erard, D. Turrini, S. Stefani, M. Amoroso, A. Olivieri
During the first orbit around Jupiter of the NASA/Juno mission, the Jovian Auroral Infrared Mapper (JIRAM) instrument observed the auroral regions with a large number of measurements. The measured spectra show both the emission of the H3+ ion and of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::dbeb623f9cedd46a9b95e5c6f0a00d11
http://hdl.handle.net/20.500.12386/30588
http://hdl.handle.net/20.500.12386/30588