F
Flora Paganelli
Researcher at Search for extraterrestrial intelligence
Publications - 59
Citations - 2829
Flora Paganelli is an academic researcher from Search for extraterrestrial intelligence. The author has contributed to research in topics: Titan (rocket family) & Radar. The author has an hindex of 20, co-authored 59 publications receiving 2608 citations. Previous affiliations of Flora Paganelli include First Green Bank & California Institute of Technology.
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Journal ArticleDOI
The lakes of Titan
Ellen R. Stofan,Charles Elachi,Jonathan I. Lunine,R. D. Lorenz,Bryan Stiles,Karl L. Mitchell,Steven J. Ostro,Laurence A. Soderblom,Charles A. Wood,Howard A. Zebker,S. D. Wall,Michael Janssen,Randolph L. Kirk,Rosaly M. C. Lopes,Flora Paganelli,Jani Radebaugh,Lauren Wye,Y. Anderson,Matthew A. Allison,R. Boehmer,Philip S. Callahan,Pierre Encrenaz,E. Flamini,G. Francescetti,Yonggyu Gim,G. Hamilton,S. Hensley,William T. K. Johnson,K. Kelleher,Duane O. Muhleman,P. Paillou,Giovanni Picardi,Francesco Posa,L. Roth,Roberto Seu,S. Shaffer,S. Vetrella,Robert West +37 more
TL;DR: These northern-hemisphere lakes constitute the strongest evidence yet that a condensable-liquid hydrological cycle is active in Titan’s surface and atmosphere, in which the lakes are filled through rainfall and/or intersection with the subsurface ‘liquid methane’ table.
Journal ArticleDOI
The sand seas of Titan: Cassini RADAR observations of longitudinal dunes.
Ralph D. Lorenz,S. D. Wall,Jani Radebaugh,G. Boubin,E. Reffet,M. A. Janssen,Ellen R. Stofan,Rosaly M. C. Lopes,Randolph L. Kirk,Charles Elachi,Jonathan I. Lunine,Jonathan I. Lunine,K. L. Mitchell,Flora Paganelli,Laurence A. Soderblom,Charles A. Wood,Lauren Wye,Howard A. Zebker,Y. Anderson,Steven J. Ostro,Matthew A. Allison,R. Boehmer,Philip S. Callahan,Pierre Encrenaz,Gian Gabriele Ori,G. Francescetti,Yonggyu Gim,G. Hamilton,Scott Hensley,William L. Johnson,K. Kelleher,Duane O. Muhleman,Giovanni Picardi,Francesco Posa,L. Roth,Roberto Seu,S. Shaffer,Bryan Stiles,S. Vetrella,Enrico Flamini,Robert West +40 more
TL;DR: The most recent Cassini RADAR images of Titan show widespread regions that appear to be seas of longitudinal dunes similar to those seen in the Namib desert on Earth, and the distribution and orientation of the dunes support a model of fluctuating surface winds.
Journal ArticleDOI
Cassini radar views the surface of Titan
Charles Elachi,S. D. Wall,Matthew A. Allison,Y. Anderson,R. Boehmer,Philip S. Callahan,Pierre Encrenaz,Enrico Flamini,Giorgio Franceschetti,Yonggyu Gim,G. Hamilton,Scott Hensley,M. A. Janssen,William L. Johnson,K. Kelleher,Randolph L. Kirk,Rosaly M. C. Lopes,Ralph D. Lorenz,Jonathan I. Lunine,Duane O. Muhleman,Steven J. Ostro,Flora Paganelli,Giovanni Picardi,Francesco Posa,L. Roth,Roberto Seu,S. Shaffer,Laurence A. Soderblom,Bryan Stiles,Ellen R. Stofan,S. Vetrella,Robert West,Charles A. Wood,Lauren Wye,Howard A. Zebker +34 more
TL;DR: The Cassini Titan Radar Mapper imaged about 1% of Titan's surface at a resolution of ∼0.5 kilometer, and larger areas of the globe in lower resolution modes, revealing a complex surface, with areas of low relief and a variety of geologic features suggestive of dome-like volcanic constructs, flows, and sinuous channels.
Journal ArticleDOI
Cryovolcanic features on Titan's surface as revealed by the Cassini Titan Radar Mapper
Rosaly M. C. Lopes,Karl L. Mitchell,Ellen R. Stofan,Jonathan I. Lunine,Jonathan I. Lunine,R. D. Lorenz,Flora Paganelli,Randolph L. Kirk,Charles A. Wood,Stephen D. Wall,L. E. Robshaw,Andrew Dominic Fortes,Catherine D. Neish,Jani Radebaugh,E. Reffet,Steven J. Ostro,Charles Elachi,Michael Allison,Y. Anderson,R. Boehmer,G. Boubin,Philip S. Callahan,Pierre Encrenaz,Enrico Flamini,G. Francescetti,Yonggyu Gim,G. Hamilton,Scott Hensley,Michael Janssen,William T. K. Johnson,K. Kelleher,Duane O. Muhleman,Gian Gabriele Ori,Roberto Orosei,Giovanni Picardi,Francesco Posa,L. Roth,Roberto Seu,S. Shaffer,Laurence A. Soderblom,Bryan Stiles,S. Vetrella,Richard West,Lauren Wye,Howard A. Zebker +44 more
TL;DR: The Cassini Titan Radar Mapper obtained Synthetic Aperture Radar images of Titan's surface during four fly-bys during the mission's first year as mentioned in this paper, showing evidence of major planetary geologic processes, including cryovolcanism.
Journal ArticleDOI
Fluvial channels on Titan: Initial Cassini RADAR observations
Ralph D. Lorenz,Rosaly M. C. Lopes,Flora Paganelli,Jonathan I. Lunine,Randolph L. Kirk,Karl L. Mitchell,L. A. Soderblom,Ellen R. Stofan,Gian Gabriele Ori,Melissa J. Myers,Hideyaki Miyamoto,Jani Radebaugh,Bryan Stiles,Stephen D. Wall,Charles A. Wood +14 more
TL;DR: Cassini radar images show a variety of fluvial channels on Titan's surface, often several hundreds of kilometers in length as mentioned in this paper, with valley widths of up to 3 kilometers across and depth of several hundred meters.