Zobrazeno 1 - 10
of 16
pro vyhledávání: '"Boris Pestoni"'
Autor:
Andrea Longobardo, Minjae Kim, Boris Pestoni, Mauro Ciarniello, Giovanna Rinaldi, Stavro Ivanovski, Fabrizio Dirri, Marco Fulle, Vincenzo Della Corte, Alessandra Rotundi, Martin Rubin
Publikováno v:
Universe, Vol 9, Iss 10, p 446 (2023)
The ESA/Rosetta mission accompanied the Jupiter Family Comet 67P/Churyumov-Gerasimenko and provided a huge amount of data which are providing important results about cometary activity mechanisms. We summarize the results obtained within the ISSI Inte
Externí odkaz:
https://doaj.org/article/8ccc9cda5b59465e89b1036d863f5f65
Autor:
Daniel Müller, Kathrin Altwegg, Jean-Jacques Berthelier, Michael Combi, Johan De Keyser, Stephen Fuselier, Boris Pestoni, Martin Rubin, Susanne Wampfler
Vincent et al. (2016) studied a 3-month period surrounding comet 67P’s perihelion passage in August 2015. They detected and characterized 34 different dust outbursts with the Rosetta cameras. The sudden and brief release of dust of such transient e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b490c78c65de0fd54fae1e0aa796d3da
https://doi.org/10.5194/epsc2022-517
https://doi.org/10.5194/epsc2022-517
Autor:
Boris Pestoni, Kathrin Altwegg, Vincenzo Della Corte, Andrea Longobardo, Daniel Müller, Alessandra Rotundi, Martin Rubin, Susanne Wampfler
The Rosetta mission of the European Space Agency has enabled a deep study of the nucleus and coma of comet 67P/Churyumov-Gerasimenko (hereafter 67P). Four instruments onboard the Rosetta spacecraft sensed coma particles ejected from the nucleus of 67
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7adf38c35a1191fe235a10af2540c30f
https://doi.org/10.5194/epsc2022-971
https://doi.org/10.5194/epsc2022-971
Autor:
Andrea Longobardo, Minjae Kim, Boris Pestoni, Hervé Cottin, Carsten Guttler, Stavro Ivanovski, Thurid Mannel, Sihane Merouane, Giovanna Rinaldi, Martin Rubin, Cecilia Tubiana, Vladimir Zakharov, Prasanna Deshapriya, Fabrizio Dirri, Mauro Ciarniello, Vincenzo Della Corte, Marco Fulle, Ernesto Palomba, Alessandra Rotundi
Introduction The ESA Rosetta mission orbited the 67P/Churyumov-Gerasimenko comet (hereafter 67P) for two years and its results are providing important clues to understand activity processes on comets. The goal of the ISSI International Team “Charac
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::928f87ae777b212e12a9c0a07e716126
https://doi.org/10.5194/epsc2022-459
https://doi.org/10.5194/epsc2022-459
Small and volatile molecules are the most abundant constituents of a comet’s neutral coma. Thanks to ESA’s Rosetta mission, the neutral coma of comet 67P/Churyumov-Gerasimenko (67P hereafter) has been analyzed in great spatial and temporal detail
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::696720e06749ed085f9fa8b37b176753
https://doi.org/10.5194/epsc2021-681
https://doi.org/10.5194/epsc2021-681
Rosetta was a mission developed by the European Space Agency aimed at the prolonged study of a remnant of the Solar System formation: the Jupiter-family comet 67P/Churyumov-Gerasimenko (hereafter, 67P). After ten years of travel, on 6 August 2014 the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::088d294541081ce2d48c0efbfb60176b
https://doi.org/10.5194/epsc2021-513
https://doi.org/10.5194/epsc2021-513
While the volatile species in comet 67P/Churyumov-Gerasimenko’s coma have been analyzed in great spatial and temporal detail, e.g., Rubin et al. (2019) or Läuter et al. (2020), little is so far known about the less volatile, heavier species. There
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::17e148f1227ce8879b30abd8b40e6cea
https://doi.org/10.5194/egusphere-egu21-1719
https://doi.org/10.5194/egusphere-egu21-1719
Autor:
Boris Pestoni, S. F. Wampfler, Martin Rubin, Isaac Schroeder, Markus Schuhmann, Hans Balsiger, Kathrin Altwegg, Nora Hänni
In an earlier study, we reported that the ram gauge of the COmet Pressure Sensor (COPS), one of the three instruments of the Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA), could be used to obtain information about the sublimating
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::71b587059f625f585f9d4cfa34780b36
Autor:
Isaac Schroeder, Kathrin Altwegg, Markus Schuhmann, Susanne F. Wampfler, Nora Hänni, Boris Pestoni, Martin Rubin
For a long time it was thought that the cyano (CN) radical, observed remotely many times in various stellar and interstellar environments, is exclusively a photodissociation product of hydrogen cyanide (HCN). Bockelée-Morvan et al. (1984) first ques
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0cd22e1dc1665428205c4c1b7ea23798
https://doi.org/10.5194/epsc2020-397
https://doi.org/10.5194/epsc2020-397
Autor:
Kathrin Altwegg, Hans Balsiger, Martin Rubin, Nora Hänni, Boris Pestoni, Isaac R. H. G. Schroeder I, Susanne F. Wampfler, Markus Schuhmann
The coma of active comets contains two essential components resulting from cometary activity: gas and dust. To investigate the latter, the Rosetta spacecraft was equipped with several instruments fully dedicated to the analysis of dust in the coma of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::631fe5717c8a22bb8944112e5c875e3b
https://doi.org/10.5194/epsc2020-635
https://doi.org/10.5194/epsc2020-635