Zobrazeno 1 - 10
of 200
pro vyhledávání: '"D. Turrini"'
Autor:
A. Mura, F. Zambon, F. Tosi, R. M. C. Lopes, J. Rathbun, M. Pettine, A. Adriani, F. Altieri, M. Ciarniello, A. Cicchetti, G. Filacchione, D. Grassi, R. Noschese, A. Migliorini, G. Piccioni, C. Plainaki, R. Sordini, G. Sindoni, D. Turrini
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 11 (2024)
Externí odkaz:
https://doaj.org/article/6fde9d5b26eb4f2ea03b2e0a680410de
Autor:
A. Mura, F. Zambon, F. Tosi, R. M. C. Lopes, J. Rathbun, M. Pettine, A. Adriani, F. Altieri, M. Ciarniello, A. Cicchetti, G. Filacchione, D. Grassi, R. Noschese, A. Migliorini, G. Piccioni, C. Plainaki, R. Sordini, G. Sindoni, D. Turrini
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 11 (2024)
We investigate the variability of the power emission of Io’s hotspots by using recent Juno/JIRAM infrared observations. The Jovian Infrared Auroral Mapper (JIRAM) is an imaging spectrometer which began observing Jupiter in August 2016. Although obs
Externí odkaz:
https://doaj.org/article/e82e1f4a081e49fe993ba3adbaf87894
Autor:
F. Zambon, A. Mura, R. M. C. Lopes, J. Rathbun, F. Tosi, R. Sordini, R. Noschese, M. Ciarniello, A. Cicchetti, A. Adriani, L. Agostini, G. Filacchione, D. Grassi, G. Piccioni, C. Plainaki, G. Sindoni, D. Turrini, S. Brooks, C. Hansen‐Koharcheck, S. Bolton
Publikováno v:
Geophysical Research Letters, Vol 50, Iss 1, Pp n/a-n/a (2023)
Abstract In this work, we present the most updated catalog of Io hot spots based on Juno/JIRAM data. We find 242 hot spots, including 23 previously undetected. Over the half of the new hot spots identified, are located at high northern and southern l
Externí odkaz:
https://doaj.org/article/301fe086a6d744a6b0c1fd10b6b425ec
Publikováno v:
Microbiologia Medica, Vol 19, Iss 2 (2004)
Externí odkaz:
https://doaj.org/article/aa47aee480604ab29a06352015174ae7
Publikováno v:
Microbiologia Medica, Vol 18, Iss 2 (2003)
Externí odkaz:
https://doaj.org/article/212d3131849140549960366393f43b0c
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 520:4683-4695
The atmospheric C/O ratio of exoplanets is widely used to constrain their formation. To guarantee that the C/O ratio provides robust information, we need to accurately quantify the amount of C and O in exoplanetary atmospheres. In the case of O, wate
Publikováno v:
Astronomy & Astrophysics.
Several science Working Groups (WG) were formed in 2019 within the Ariel Mission Consortium to help prepare the RedBook (Tinetti et al. ESA/SCI(2020)1), defining the science cases, and to contribute to address three fundamental questions 1) what exop
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3277fa4e8bb44526c494da347379f48d
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Autor:
A. Suárez Mascareño, M. Damasso, N. Lodieu, A. Sozzetti, V. J. S. Béjar, S. Benatti, M. R. Zapatero Osorio, G. Micela, R. Rebolo, S. Desidera, F. Murgas, R. Claudi, J. I. González Hernández, L. Malavolta, C. del Burgo, V. D’Orazi, P. J. Amado, D. Locci, H. M. Tabernero, F. Marzari, D. S. Aguado, D. Turrini, C. Cardona Guillén, B. Toledo-Padrón, A. Maggio, J. Aceituno, F. F. Bauer, J. A. Caballero, P. Chinchilla, E. Esparza-Borges, E. González-Álvarez, T. Granzer, R. Luque, E. L. Martín, G. Nowak, M. Oshagh, E. Pallé, H. Parviainen, A. Quirrenbach, A. Reiners, I. Ribas, K. G. Strassmeier, M. Weber, M. Mallonn
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
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Current theories of planetary evolution predict that infant giant planets have large radii and very low densities before they slowly contract to reach their final size after about several hundred million years1,2. These theoretical expectations remai