Zobrazeno 1 - 10 of 60 pro vyhledávání: '"M. Salatti"'
1
Cometary coma dust size distribution from in situ IR spectra
Autor: Stefano Mottola, Giovanna Rinaldi, Stéphane Erard, Marco Fulle, Andrea Longobardo, M. Salatti, Maria Teresa Capria, Fredric W. Taylor, Alessandra Rotundi, Stavro Ivanovski, Dominique Bockelée-Morvan, G. P. Tozzi, Ernesto Palomba, Mauro Ciarniello, V. Della Corte, Gianrico Filacchione, C. Leyrat, Fabrizio Capaccioni, Emiliano D'Aversa
Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 469 (Suppl_2), pp.S598-S605. ⟨10.1093/mnras/stx1873⟩
Monthly Notices of the Royal Astronomical Society, 2017, 469 (Suppl_2), pp.S598-S605. ⟨10.1093/mnras/stx1873⟩
Dust is the most abundant component in cometary comae. Here, we investigate the dust size distribution in 67P/Churyumov-Gerasimenko (67P/CG) using data from the Rosetta spacecraft that was in close proximity to the comet from 2014 August to 2016 Sept
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fc195391b72a0c6b0f68c1fcb97e78ac
https://doi.org/10.1093/mnras/stx1873
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2
Akademický článek
Differential kinetic dynamics and heating of ions in the turbulent solar wind
Autor: F Valentini, D Perrone, S Stabile, O Pezzi, S Servidio, R De Marco, F Marcucci, R Bruno, B Lavraud, J De Keyser, G Consolini, D Brienza, L Sorriso-Valvo, A Retinò, A Vaivads, M Salatti, P Veltri
Publikováno v: New Journal of Physics, Vol 18, Iss 12, p 125001 (2016)
The solar wind plasma is a fully ionized and turbulent gas ejected by the outer layers of the solar corona at very high speed, mainly composed by protons and electrons, with a small percentage of helium nuclei and a significantly lower abundance of h
Externí odkaz: https://doaj.org/article/9ac42af10ea24b5d8634d6953101a690
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3
The Solar Orbiter Solar Wind Analyser (SWA) suite
Autor: C. Brockley-Blatt, Mark Phillips, G. Dirks, A. Malpus, J. Ford, Michael R. Collier, M. Hailey, C. Loeffler, G. Terrier, S. Myers, Iannis Dandouras, D. Rust, G. Capuano, L. M. Kistler, Gethyn R. Lewis, S. Clemens, R. Baruah, John A. Trevino, R. Ascolese, Jean-André Sauvaud, S. Persyn, K. Ruane, C. Urdiales, E. Penou, G. Davison, Timothy J. Stubbs, A. Barthe, J. Yardley, Vincent Génot, A. Lawrenson, R. Thibodeaux, B. Hancock, Glyn Collinson, Jason A. Gilbert, C. Anekallu, C. Jacquey, Robert F. Wimmer-Schweingruber, I. Čermák, S. Gradone, L. Přech, J. Coker, P. Louarn, V. de Giosa, Berend Winter, Timothy S. Horbury, W. Marty, M. Salatti, Daniel Verscharen, Jim M. Raines, P. Devoto, E. Edlund, C. Brysbaert, M. Johnson, J. Rubiella, T. Hunt, Frederic Allegrini, M. Ferris, Roberto Bruno, Matthieu Berthomier, M. Petiot, Christopher J. Owen, K. L. Arnett, A. Rousseau, D. Davies, V. Arciuli, P. Bland, Peter Wurz, J. W. Thomas, G. Mele, R. Calvanese, G. Watson, F. Monti, C. Bancroft, Dennis J. Chornay, P. Wheeler, Andrew Walsh, Jason L. Stange, K. Al Janabi, Dhiren Kataria, V. Fortunato, Keiichi Ogasawara, A. Spencer, Rossana DeMarco, Susan T. Lepri, C. Amoros, Milan Maksimovic, D. Heirtzler, Stefano Livi, N. André, Antoinette B. Galvin, Mark A. Popecki, Benoit Lavraud, A. Alapide, W. Gibson, Leonardo Amoruso, W. Lockhart, Raffaella D'Amicis, G. Willis, C. Mazelle, F. Marcucci, S. Rogacki, A. Pacros, A. P. Rouillard, F. Leblanc, K. Rees, J.-D. Techer, Javier Rodriguez-Pacheco, I. Fratter, Ali Varsani, I. Zouganelis, M. Orlandi, C. Garat, T. Taylor, Marco Castronuovo, C. Frost, G. Fruit, A. De Los Santos, A. Mayall, M. Reden, Andrew Fazakerley, R. Mathon, I. Phillips, A. Fedorov, T. Nguyen, H. Seran, M. Brysch, R. Darnley, Mark Stakhiv, S. Bordon
Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 642, pp.A16. ⟨10.1051/0004-6361/201937259⟩
Astronomy and Astrophysics-A&A, 2020, 642, pp.A16. ⟨10.1051/0004-6361/201937259⟩
The Solar Orbiter mission seeks to make connections between the physical processes occurring at the Sun or in the solar corona and the nature of the solar wind created by those processes which is subsequently observed at the spacecraft. The mission a
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::610f9db9949bdb85fca0d7ab9f5aea86
https://hal-cnrs.archives-ouvertes.fr/hal-03006485/file/aa37259-19.pdf
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4
GIADA microbalance measurements on board Rosetta: Submicrometer- To micrometer-sized dust particle flux in the coma of comet 67P/Churyumov-Gerasimenko
Autor: Pasquale Palumbo, Andrea Longobardo, M. Salatti, Stavro Ivanovski, V. Zakharov, Z. Dionnet, Alessandra Rotundi, Vito Liuzzi, V. Della Corte, Marco Fulle
Context. From August 2014 to September 2016, Rosetta escorted comet 67P/Churyumov-Gerasimenko (67P) during its journey around the Sun. One of the aims of Rosetta was to characterize cometary activity and the consequent formation of dust flux structur
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::98641b4c0ba32f408e712c074f17398d
http://hdl.handle.net/11367/90993
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5
Summer outbursts in the coma of comet 67P/Churyumov-Gerasimenko as observed by Rosetta-VIRTIS
Autor: David Kappel, Fabrizio Capaccioni, Dominique Bockelée-Morvan, Uwe Fink, Andrea Raponi, Stéphane Erard, V. Della Corte, Gianrico Filacchione, Andrea Longobardo, Alessandra Rotundi, M. T. Capria, Giovanna Rinaldi, M. Salatti, G. P. Tozzi, Alessandra Migliorini, Fredric W. Taylor, Federico Tosi, C. Leyrat, Ernesto Palomba, Mauro Ciarniello, Emiliano D'Aversa, S. Ivanovski, Lyn R. Doose
Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 481 (1), pp.1235-1250. ⟨10.1093/mnras/sty2266⟩
We present an analysis of transient events observed by the Visible InfraRed Thermal Imaging Spectrometer, instrument aboard Rosetta, for the dates of 2015 August 10, September 13 and 14, during the two months surrounding the comet perihelion passage
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::868a25a1a3f79031c211543acdfc8462
https://elib.dlr.de/124868/
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6
The global surface composition of 67P/Churyumov-Gerasimenko nucleus by Rosetta/VIRTIS. II) Diurnal and seasonal variability
Autor: M. A. Barucci, Stefano Mottola, Alessandra Migliorini, Federico Tosi, Gabriele Arnold, Priscilla Cerroni, Andrea Longobardo, M. T. Capria, Giovanna Rinaldi, M. Salatti, Bernard Schmitt, Andrea Raponi, W-H. Ip, Angelo Zinzi, Mauro Ciarniello, C. Leyrat, Giuseppe Piccioni, Batiste Rousseau, David Kappel, Fabrizio Capaccioni, Eric Quirico, Stéphane Erard, Gianrico Filacchione, Ernesto Palomba, E. Kuehrt, D. Bockelee-Morvan, M.C. Desanctis
Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2016, 462 (Issue Suppl_1), pp.S443-S458. ⟨10.1093/mnras/stw3177⟩
Monthly Notices of the Royal Astronomical Society, 2016, 462 (Issue Suppl_1), pp.S443-S458. ⟨10.1093/mnras/stw3177⟩
International audience; VIRTIS-M observations of the nucleus of comet 67P/Churyumov-Gerasimenko acquired from 2014 August to 2015 May have been analysed to investigate surface temporal variability at both seasonal and diurnal scales. The measured ref
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d898fb378b925fb7d4a7c5d1b2decff8
https://doi.org/10.1093/mnras/stw3177
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7
Importance of energy and angular resolutions in top-hat electrostatic analysers for solar wind proton measurements
Autor: Sergio Servidio, R. De Marco, Francesco Valentini, M. Salatti, Roberto Bruno, Raffaella D'Amicis, Benoit Lavraud, Maria Federica Marcucci, Philippe Louarn
We use a numerical code which reproduces the angular/energy response of a typical top-hat electrostatic analyser starting from solar wind proton velocity distribution functions (VDFs) generated by numerical simulations. The simulations are based on t
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1fdd33764ec55142323dfbd4a47d7979
http://hdl.handle.net/20.500.12386/26453
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8
Differential kinetic dynamics and heating of ions in the turbulent solar wind
Autor: M. Salatti, Francesco Valentini, Sergio Servidio, Giuseppe Consolini, Andris Vaivads, Daniele Brienza, Benoit Lavraud, S. Stabile, Pierluigi Veltri, F. Marcucci, Luca Sorriso-Valvo, Denise Perrone, Alessandro Retinò, R. De Marco, Oreste Pezzi, Roberto Bruno, J. De Keyser
Publikováno v: New Journal of Physics
New Journal of Physics, Institute of Physics: Open Access Journals, 2016, 18, pp.125001. ⟨10.1088/1367-2630/18/12/125001⟩
New Journal of Physics, 2016, 18, pp.125001. ⟨10.1088/1367-2630/18/12/125001⟩
International audience; The solar wind plasma is a fully ionized and turbulent gas ejected by the outer layers of the solar corona at very high speed, mainly composed by protons and electrons, with a small percentage of helium nuclei and a significan
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1bf75f34478e34288fe490bbb3283171
https://hal.archives-ouvertes.fr/hal-01551963
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9
A multiple-rendezvous, sample-return mission to two near-Earth asteroids
Autor: Rene Duffard, S. Arloth, S. Pirrotta, M. Salatti, A. Duricic, U. Derz, S. Poulsen, R. M. G. Armytage, Jessica Flahaut, K. Kumar, L. Donati, M. Kubínyi, A. Pollinger, Stefanie Hempel
Publikováno v: Advances in Space Research
Advances in Space Research, Elsevier, 2011, 48 (1), pp.120-132. ⟨10.1016/j.asr.2011.02.013⟩
Advances in Space Research, 2011, 48 (1), pp.120-132. ⟨10.1016/j.asr.2011.02.013⟩
International audience; We propose a dual-rendezvous mission, targeting near-Earth asteroids, including sample-return. The mission, Asteroid Sampling Mission (ASM), consists of two parts: (i) flyby and remote sensing of a Q-type asteroid, and (ii) sa
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::07fbc375d375c74ef01e628fdde60c5d
https://hal.archives-ouvertes.fr/hal-00661136
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10
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