Zobrazeno 1 - 10
of 59
pro vyhledávání: '"Hsiang-Wen Hsu"'
Autor:
Xin Cao, Xiangning Chu, Hsiang-Wen Hsu, Hao Cao, Weijie Sun, Lucas Liuzzo, Jasper Halekas, Carol Paty, Feng Chu, Omakshi Agiwal, Lauren Blum, Frank Crary, Ian J. Cohen, Peter Delamere, Mark Hofstadter, George Hospodarsky, Cooper John, Peter Kollmann, Elena Kronberg, William Kurth, Laurent Lamy, Dong Lin, Wen Li, Xuanye Ma, David Malaspina, Michiko Morooka, Tom Nordheim, Frank Postberg, Andrew Poppe, Cartwright Richard, Suranga Ruhunusiri, Krista Soderlund, James O'Donoghue, Ferdinand Plaschke
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 11 (2024)
The magnetospheric systems of ice giants, as the ideal and the unique template of a typical class of exoplanets, have not been sufficiently studied in the past decade. The complexity of these asymmetric and extremely dynamic magnetospheres provides u
Externí odkaz:
https://doaj.org/article/8463fd388762420fa033023837f113ca
Autor:
Omakshi Agiwal, Hao Cao, Hsiang-Wen Hsu, Luke Moore, Ali H. Sulaiman, James O’Donoghue, Michele K. Dougherty
Publikováno v:
The Planetary Science Journal, Vol 5, Iss 6, p 134 (2024)
This study presents a synthesized analysis of in situ and ground-based observations to investigate electromagnetic coupling between Saturn and its rings. During the Cassini Grand Finale, the magnetometer detected gradients in the azimuthal magnetic f
Externí odkaz:
https://doaj.org/article/4a50c86485294026bfc95ea5ed2a4059
Publikováno v:
Universe, Vol 8, Iss 5, p 261 (2022)
Europa has been spotted as having water outgassing activities by space- and ground-based telescopes as well as reanalysis of the Galileo data. We adopt a 3D Direct Simulation Monte Carlo (DSMC) model to investigate the observed plume characteristics
Externí odkaz:
https://doaj.org/article/7541da83a2174a90a7669fa0e0ee8c1c
Publikováno v:
Nature Astronomy. 6:1043-1050
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d001eead84def1b438c129b4c423edbc
https://doi.org/10.1038/s41550-022-01717-9
https://doi.org/10.1038/s41550-022-01717-9
Space missions often carry antenna instruments that are sensitive to dust impacts, however, the understanding of signal generation mechanisms remained incomplete. A signal generation model in an analytical form is presented that provides a good agree
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::87c1be334ef525872cff5a1637bcbea0
Autor:
Simon Linti, Hsiang-Wen Hsu, Christian Fischer, Mario Trieloff, Jon Hillier, Juergen Schmidt, Frank Postberg
Measurements during the final phase of the Cassini mission revealed the composition of individual dust particles, ejected by micrometeoroid impacts from Saturn’s main rings. These measurements were conducted with the in situ time-of-flight mass spe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ef0e6a6731fe427bd1d3d0846aa4134a
https://doi.org/10.5194/epsc2022-367
https://doi.org/10.5194/epsc2022-367
Autor:
Matthew H. Burger, V. Mangano, Cesare Grava, Hsiang-Wen Hsu, Nicholas M. Schneider, Kurt D. Retherford, François Leblanc, Timothy A. Cassidy, Jeffrey P. Morgenthaler, Cesare Barbieri
Publikováno v:
The Astronomical Journal
The Astronomical Journal, American Astronomical Society, 2021, 162 (5), pp.190. ⟨10.3847/1538-3881/ac1ff8⟩
The Astronomical Journal, American Astronomical Society, 2021, 162 (5), pp.190. ⟨10.3847/1538-3881/ac1ff8⟩
International audience; We report the results of model simulations performed to explain the nature of a sodium emission feature in Io Neutral Clouds. The feature was detected via high-resolution spectroscopic observations from the 3.6 m Italian teles
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2ee6c7c148fd864c02f8982077d30594
https://hal-insu.archives-ouvertes.fr/insu-03374890/file/GravaAJ2021.pdf
https://hal-insu.archives-ouvertes.fr/insu-03374890/file/GravaAJ2021.pdf
During the final mission phase, the Cassini spacecraft travelled through the gap between Saturn and its innermost D ring. One goal of these highly inclined orbits was sampling the dust population, mostly made of impact ejecta from the main rings, in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::30a2fb9c6ec055b3732fa44a20bdc091
https://doi.org/10.5194/epsc2021-181
https://doi.org/10.5194/epsc2021-181
Publikováno v:
Nature Astronomy. 3:967-970
Spectacular results from Cassini’s Grand Finale have provided constraints on the characteristics and evolutionary processes of Saturn’s rings. These results have been interpreted as proof that the rings are much younger than the Solar System, dra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d6c16b5a2a42bbbad0d4e83ff6bd703e
https://doi.org/10.1038/s41550-019-0876-y
https://doi.org/10.1038/s41550-019-0876-y