S
Stefano Debei
Researcher at University of Padua
Publications - 290
Citations - 10185
Stefano Debei is an academic researcher from University of Padua. The author has contributed to research in topics: Comet & Field of view. The author has an hindex of 47, co-authored 286 publications receiving 8851 citations. Previous affiliations of Stefano Debei include University of Trento.
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Journal ArticleDOI
In situ measurements of the physical characteristics of Titan's environment
Marcello Fulchignoni,Francesca Ferri,Francesco Angrilli,Andrew J. Ball,Akiva Bar-Nun,M. A. Barucci,C. Bettanini,G. Bianchini,William J. Borucki,Giacomo Colombatti,M. Coradini,Athena Coustenis,Stefano Debei,Peter Falkner,Giulio Fanti,Enrico Flamini,V. Gaborit,R. Grard,Michel Hamelin,Ari-Matti Harri,B. Hathi,Irmgard Jernej,Mark Leese,A. Lehto,P. F. Lion Stoppato,J. J. López-Moreno,T. Mäkinen,J. A. M. McDonnell,Christopher P. McKay,Gregorio J. Molina-Cuberos,Fritz M. Neubauer,Valerio Pirronello,Rafael Rodrigo,Bortolino Saggin,Konrad Schwingenschuh,Alvin Seiff,Fernando Simões,Håkan Svedhem,Tetsuya Tokano,Martin C. Towner,R. Trautner,Paul Withers,Paul Withers,John C. Zarnecki +43 more
TL;DR: The temperature and density profiles, as determined by the Huygens Atmospheric Structure Instrument (HASI), from an altitude of 1,400 km down to the surface were higher than expected and the extent of atmospheric electricity was also hitherto unknown.
Journal ArticleDOI
On the nucleus structure and activity of comet 67P/Churyumov-Gerasimenko
Holger Sierks,Cesare Barbieri,Philippe Lamy,Rafael Rodrigo,Rafael Rodrigo,Detlef Koschny,Hans Rickman,H. U. Keller,H. U. Keller,Jessica Agarwal,Michael F. A'Hearn,Michael F. A'Hearn,Francesco Angrilli,A.-T. Auger,M. Antonella Barucci,Jean-Loup Bertaux,Ivano Bertini,Sebastien Besse,Dennis Bodewits,Claire Capanna,Gabriele Cremonese,Vania Da Deppo,Bjö Davidsson,Stefano Debei,Mariolino De Cecco,Francesca Ferri,Sonia Fornasier,Marco Fulle,Robert Gaskell,Lorenza Giacomini,Olivier Groussin,P. Gutierrez-Marques,Pedro J. Gutiérrez,Carsten Güttler,N. M. Hoekzema,Stubbe F. Hviid,Stubbe F. Hviid,Wing-Huen Ip,Wing-Huen Ip,Laurent Jorda,Jörg Knollenberg,Gábor L. Kovács,J. Rainer Kramm,Ekkehard Kührt,Michael Küppers,Fiorangela La Forgia,Luisa Lara,Monica Lazzarin,C. Leyrat,Jose J. Lopez Moreno,Sara Magrin,Simone Marchi,Francesco Marzari,Matteo Massironi,Harald Michalik,Richard Moissl,Stefano Mottola,Giampiero Naletto,Nilda Oklay,Maurizio Pajola,Marco Pertile,Frank Preusker,L. Sabau,Frank Scholten,Colin Snodgrass,Nicolas Thomas,Cecilia Tubiana,Jean-Baptiste Vincent,Klaus Peter Wenzel,Mirco Zaccariotto,Martin Pätzold +70 more
TL;DR: Images from the OSIRIS scientific imaging system onboard Rosetta show that the nucleus of 67P/Churyumov-Gerasimenko consists of two lobes connected by a short neck, which raises the question of whether the two Lobes represent a contact binary formed 4.5 billion years ago, or a single body where a gap has evolved via mass loss.
Journal ArticleDOI
Dust measurements in the coma of comet 67P/Churyumov-Gerasimenko inbound to the Sun
Alessandra Rotundi,Alessandra Rotundi,Holger Sierks,Vincenzo Della Corte,Marco Fulle,Pedro J. Gutiérrez,Luisa Lara,Cesare Barbieri,Philippe Lamy,Rafael Rodrigo,Rafael Rodrigo,Detlef Koschny,Hans Rickman,Hans Rickman,H. U. Keller,José Juan López-Moreno,Mario Accolla,Mario Accolla,Jessica Agarwal,Michael F. A'Hearn,Nicolas Altobelli,Francesco Angrilli,M. Antonietta Barucci,Jean-Loup Bertaux,Ivano Bertini,Dennis Bodewits,E. Bussoletti,Luigi Colangeli,M. Cosi,Gabriele Cremonese,Jean-François Crifo,Vania Da Deppo,Björn Davidsson,Stefano Debei,Mariolino De Cecco,Francesca Esposito,M. Ferrari,M. Ferrari,Sonia Fornasier,F. Giovane,Bo Å. S. Gustafson,Simon F. Green,Olivier Groussin,Eberhard Grün,Carsten Güttler,M. Herranz,Stubbe F. Hviid,Wing Ip,Stavro Ivanovski,José M. Jerónimo,Laurent Jorda,J. Knollenberg,R. Kramm,Ekkehard Kührt,Michael Küppers,Monica Lazzarin,Mark Leese,Antonio C. López-Jiménez,F. Lucarelli,Stephen C. Lowry,Francesco Marzari,Elena Mazzotta Epifani,J. Anthony M. McDonnell,J. Anthony M. McDonnell,Vito Mennella,Harald Michalik,A. Molina,R. Morales,Fernando Moreno,Stefano Mottola,Giampiero Naletto,Nilda Oklay,Jose Luis Ortiz,Ernesto Palomba,Pasquale Palumbo,Pasquale Palumbo,Jean-Marie Perrin,Jean-Marie Perrin,J. E. Rodriguez,L. Sabau,Colin Snodgrass,Colin Snodgrass,Roberto Sordini,Nicolas Thomas,Cecilia Tubiana,Jean-Baptiste Vincent,Paul R. Weissman,K. P. Wenzel,Vladimir Zakharov,John C. Zarnecki,John C. Zarnecki +90 more
TL;DR: In this article, the GIADA (Grain Impact Analyser and Dust Accumulator) experiment on the European Space Agency's Rosetta spacecraft orbiting comet 67P/Churyumov-Gerasimenko was used to detect 35 outflowing grains of mass 10−10 to 10−7 kilograms.
Journal ArticleDOI
OSIRIS – The Scientific Camera System Onboard Rosetta
H. U. Keller,Cesare Barbieri,Philippe Lamy,Hans Rickman,Rafael Rodrigo,K.-P. Wenzel,Holger Sierks,Michael F. A'Hearn,Francesco Angrilli,M. Angulo,M. E. Bailey,Peter Barthol,M. A. Barucci,Jean-Loup Bertaux,G. Bianchini,J.-L. Boit,V. Brown,Joseph A. Burns,I. Büttner,José María Bermúdez de Castro,Gabriele Cremonese,Gabriele Cremonese,Werner Curdt,V. Da Deppo,Stefano Debei,M. De Cecco,M. De Cecco,Kjetil Dohlen,Sonia Fornasier,Marco Fulle,D. Germerott,Fritz Gliem,Gian Paolo Guizzo,Stubbe F. Hviid,Wing-Huen Ip,Laurent Jorda,Detlef Koschny,J.-R. Kramm,Ekkehard Kührt,Michael Küppers,Luisa Lara,A. Llebaria,A. López,A. Lopez-Jimenez,J. J. López-Moreno,R. Meller,Harald Michalik,M. D. Michelena,R. Muller,Giampiero Naletto,Alain Origne,G. Parzianello,Marco Pertile,C. Quintana,Roberto Ragazzoni,Roberto Ragazzoni,P. Ramous,K.-U. Reiche,M. Reina,J. E. Rodriguez,Gérard Rousset,L. Sabau,A. Sanz,Jean-Pierre Sivan,K. Stöckner,J. Tabero,U. Telljohann,Nicolas Thomas,V. Timon,G. Tomasch,T. Wittrock,Mirco Zaccariotto +71 more
TL;DR: The Optical, Spectroscopic, and Infrared Remote Imaging System (OSIRIS) as discussed by the authors is the scientific camera system onboard the Rosetta spacecraft, which consists of a high resolution Narrow Angle Camera (NAC) and a wide angle Camera (WAC) units accompanied by three electronics boxes.
Journal ArticleDOI
The morphological diversity of comet 67P/Churyumov-Gerasimenko
Nicolas Thomas,Holger Sierks,Cesare Barbieri,Philippe Lamy,Rafael Rodrigo,Hans Rickman,Detlef Koschny,H. U. Keller,H. U. Keller,Jessica Agarwal,Michael F. A'Hearn,Francesco Angrilli,A.-T. Auger,M. Antonella Barucci,Jean-Loup Bertaux,Ivano Bertini,Sebastien Besse,Dennis Bodewits,Gabriele Cremonese,Vania Da Deppo,B. J. R. Davidsson,Mariolino De Cecco,Stefano Debei,Mohamed Ramy El-Maarry,Francesca Ferri,Sonia Fornasier,Marco Fulle,Lorenza Giacomini,Olivier Groussin,Pedro J. Gutiérrez,Carsten Güttler,Stubbe F. Hviid,Wing-Huen Ip,Laurent Jorda,J. Knollenberg,J. Rainer Kramm,Ekkehard Kührt,Michael Küppers,Fiorangela La Forgia,Luisa Lara,Monica Lazzarin,Jose J. Lopez Moreno,Sara Magrin,Simone Marchi,Francesco Marzari,Matteo Massironi,Harald Michalik,Richard Moissl,Stefano Mottola,Giampiero Naletto,Nilda Oklay,Maurizio Pajola,Antoine Pommerol,Frank Preusker,L. Sabau,Frank Scholten,Colin Snodgrass,Cecilia Tubiana,Jean-Baptiste Vincent,K. P. Wenzel +59 more
TL;DR: Images of comet 67P/Churyumov-Gerasimenko acquired by the OSIRIS imaging system onboard the European Space Agency’s Rosetta spacecraft offer some support for subsurface fluidization models and mass loss through the ejection of large chunks of material.