D
Darrell F. Strobel
Researcher at Johns Hopkins University
Publications - 335
Citations - 16986
Darrell F. Strobel is an academic researcher from Johns Hopkins University. The author has contributed to research in topics: Atmosphere & Jupiter. The author has an hindex of 68, co-authored 328 publications receiving 15856 citations. Previous affiliations of Darrell F. Strobel include Johns Hopkins University Applied Physics Laboratory & United States Naval Research Laboratory.
Papers
More filters
Journal ArticleDOI
Extreme ultraviolet observations from Voyager 1 encounter with Jupiter
A. L. Broadfoot,M. J. S. Belton,P. Z. Takacs,Bill R. Sandel,Donald E. Shemansky,Jay B. Holberg,Joseph M. Ajello,Sushil K. Atreya,Thomas M. Donahue,H. W. Moos,Jean-Loup Bertaux,J. E. Blamont,Darrell F. Strobel,John C. McConnell,Alexander Dalgarno,Richard Goody,Michael B. McElroy +16 more
TL;DR: The observed resonance scattering of solar hydrogen Lyman α by the atmosphere of Jupiter and the solar occultation experiment suggest a hot thermosphere (≥ 1000 K) wvith a large atomic hydrogen abundance.
Journal ArticleDOI
Transient Water Vapor at Europa’s South Pole
Lorenz Roth,Lorenz Roth,Joachim Saur,Kurt D. Retherford,Darrell F. Strobel,Paul D. Feldman,Melissa A. McGrath,Francis Nimmo +7 more
TL;DR: Europa's Plumes Jupiter's moon Europa has a subsurface ocean and a relatively young icy surface, and spectral images taken by the Hubble Space Telescope show ultraviolet emissions from the moon's atmosphere that are consistent with two 200-km-high plumes of water vapor.
Journal ArticleDOI
The Pluto system: Initial results from its exploration by New Horizons.
S. A. Stern,Fran Bagenal,Kimberly Ennico,G. R. Gladstone,William M. Grundy,William B. McKinnon,J. M. Moore,Catherine B. Olkin,John R. Spencer,Harold A. Weaver,Leslie A. Young,Tom Andert,Jane M. Andrews,M. E. Banks,B. Bauer,Jeremy Bauman,Olivier S. Barnouin,Peter D. Bedini,K. B. Beisser,Ross A. Beyer,S. Bhaskaran,Richard P. Binzel,Emma Birath,Mike Bird,D. J. Bogan,Alice Bowman,Veronica J. Bray,M. Brozovic,C. Bryan,Matthew R. Buckley,Marc W. Buie,Bonnie J. Buratti,Stewart Bushman,Andrew B. Calloway,Brian Carcich,Andrew F. Cheng,Steven J. Conard,C. A. Conrad,Jason C. Cook,Dale P. Cruikshank,O. S. Custodio,C. M. Dalle Ore,C. C. Deboy,Zach Dischner,Philip J. Dumont,Alissa M. Earle,H. A. Elliott,J. Ercol,Carolyn M. Ernst,Tiffany J. Finley,Sarah H. Flanigan,Glen H. Fountain,M. J. Freeze,Thomas K. Greathouse,James L. Green,Yanping Guo,Matthias Hahn,Douglas P. Hamilton,Sarah A. Hamilton,Jennifer Hanley,A. Harch,H. M. Hart,Chris B. Hersman,A. Hill,Matthew E. Hill,David P. Hinson,Mark E. Holdridge,Mihaly Horanyi,Alan D. Howard,Carly Howett,Coralie D. Jackman,Robert A. Jacobson,D. E. Jennings,Joshua A. Kammer,H. K. Kang,David E. Kaufmann,Peter Kollmann,Stamatios M. Krimigis,David Y. Kusnierkiewicz,Tod R. Lauer,J. E. Lee,K. L. Lindstrom,Ivan Linscott,Carey M. Lisse,Allen W. Lunsford,V. A. Mallder,Nicole Martin,David J. McComas,Ralph L. McNutt,Douglas S. Mehoke,Thomas Mehoke,E. D. Melin,Max Mutchler,Derek S. Nelson,Francis Nimmo,Jorge I. Nunez,A. C. Ocampo,William M. Owen,Martin Paetzold,B. Page,Alex Parker,Joel Wm. Parker,Frederic Pelletier,J. Peterson,Nickalaus Pinkine,M. Piquette,Simon B. Porter,Silvia Protopapa,Jillian Redfern,Harold J. Reitsema,D. C. Reuter,James H. Roberts,Stuart J. Robbins,Gabe Rogers,Debi Rose,Kirby Runyon,Kurt D. Retherford,M. G. Ryschkewitsch,Paul M. Schenk,Eric Schindhelm,B. Sepan,Mark R. Showalter,Kelsi N. Singer,M. Soluri,Dale Stanbridge,Andrew J. Steffl,Darrell F. Strobel,T. Stryk,Michael E. Summers,Jamey Szalay,M. B. Tapley,A. Taylor,H. W. Taylor,Henry B. Throop,Constantine Tsang,G. L. Tyler,Orkan M. Umurhan,A. J. Verbiscer,M. H. Versteeg,Michael Vincent,R. W. Webbert,S. Weidner,G. Weigle,Oliver L. White,Karl Whittenburg,B. G. Williams,Kaj E. Williams,S. P. Williams,W. W. Woods,Amanda M. Zangari,Eric J. Zirnstein +150 more
TL;DR: The New Horizons encounter revealed that Pluto displays a surprisingly wide variety of geological landforms, including those resulting from glaciological and surface-atmosphere interactions as well as impact, tectonic, possible cryovolcanic, and mass-wasting processes.
Journal ArticleDOI
Detection of an oxygen atmosphere on Jupiter's moon Europa
TL;DR: The detection of atomic oxygen emission from Europa is reported, which is interpreted as being produced by the simultaneous dissociation and excitation of atmospheric O2 by electrons from Jupiter's magnetosphere.
Journal ArticleDOI
Titan's atmospheric temperatures, winds, and composition
F. M. Flasar,R. K. Achterberg,Barney J. Conrath,Peter J. Gierasch,V. G. Kunde,Conor A. Nixon,Gordon L. Bjoraker,D. E. Jennings,Paul N. Romani,Amy A. Simon-Miller,Bruno Bézard,Athena Coustenis,Pgj Irwin,Nicholas A Teanby,John C. Brasunas,John C. Pearl,M. E. Segura,Ronald Carlson,A. A. Mamoutkine,Paul J. Schinder,Antonella Barucci,Regis Courtin,Thierry Fouchet,Daniel Gautier,Emmanuel Lellouch,A. Marten,R. Prangé,Sandrine Vinatier,Darrell F. Strobel,S. B. Calcutt,Peter L. Read,Fredric W. Taylor,Neil Bowles,Robert E. Samuelson,Glenn S. Orton,Linda Spilker,Tobias Owen,John R. Spencer,Mark R. Showalter,C. Ferrari,Mian M. Abbas,François Raulin,Scott G. Edgington,Peter A. R. Ade,E. H. Wishnow +44 more
TL;DR: Early Cassini infrared observations of Titan show a stratopause at an altitude of 310 kilometers (and 186 kelvin at 15°S), and the concentrations of several stratospheric organic compounds are enhanced at mid- and high northern latitudes, and the strong zonal winds may inhibit mixing between these latitudes and the rest of Titan.