J
J. P. Cravens
Researcher at Southwest Research Institute
Publications - 12
Citations - 825
J. P. Cravens is an academic researcher from Southwest Research Institute. The author has contributed to research in topics: Telescope & Compton telescope. The author has an hindex of 6, co-authored 12 publications receiving 692 citations.
Papers
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Journal ArticleDOI
Science Goals and Overview of the Radiation Belt Storm Probes (RBSP) Energetic Particle, Composition, and Thermal Plasma (ECT) Suite on NASA’s Van Allen Probes Mission
Harlan E. Spence,Geoffrey D. Reeves,Daniel N. Baker,J. B. Blake,M. Bolton,Sebastien Bourdarie,Anthony A. Chan,Seth G. Claudepierre,J. H. Clemmons,J. P. Cravens,Scot R. Elkington,J. F. Fennell,Reiner Friedel,Herbert O. Funsten,Jerry Goldstein,Janet C. Green,A. A. Guthrie,Michael G. Henderson,Richard B. Horne,Mary K. Hudson,J.-M. Jahn,Vania K. Jordanova,Shrikanth Kanekal,B. W. Klatt,B. W. Klatt,Brian A. Larsen,Xinlin Li,Elizabeth MacDonald,Ian R. Mann,J. T. Niehof,T. P. O'Brien,Terrance Onsager,D. Salvaggio,Ruth M. Skoug,S. Smith,L. L. Suther,Michelle F. Thomsen,Richard M. Thorne +37 more
TL;DR: The Radiation Belt Storm Probes (RBSP)-Energetic Particle, Composition, and Thermal Plasma (ECT) suite contains an innovative complement of particle instruments to ensure the highest quality measurements ever made in the inner magnetosphere and radiation belts as mentioned in this paper.
Journal ArticleDOI
The Ultraviolet Spectrograph on NASA’s Juno Mission
G. Randall Gladstone,S. Persyn,John S. Eterno,Brandon Walther,David C. Slater,Michael W. Davis,Maarten H. Versteeg,K. B. Persson,Michael K. Young,G. Dirks,Anthony O. Sawka,Jessica Tumlinson,Henry Sykes,John Beshears,Cherie L. Rhoad,J. P. Cravens,Gregory S. Winters,Robert Klar,Walter L. Lockhart,Benjamin M. Piepgrass,Thomas K. Greathouse,B. Trantham,Philip M. Wilcox,Matthew W. Jackson,Oswald H. W. Siegmund,John V. Vallerga,R. Raffanti,Adrian Martin,Jean-Claude Gérard,Denis Grodent,Bertrand Bonfond,Benoit Marquet,François Denis +32 more
TL;DR: Juno-UVS as mentioned in this paper is a long-slit imaging spectrograph designed to observe and characterize Jupiter's far-ultraviolet (FUV) auroral emissions, which are coordinated and correlated with those from other remote sensing instruments and used to place in situ measurements made by Juno's particles and fields instruments into a global context, relating the local data with events occurring in more distant regions of Jupiter's magnetosphere.
Book ChapterDOI
Medium Energy Neutral Atom (MENA) Imager for the Image Mission
C. J. Pollock,Kazushi Asamura,J. R. Baldonado,Matthew M. Balkey,P. Barker,James L. Burch,Eric J. Korpela,J. P. Cravens,G. Dirks,M.-C. Fok,Herbert O. Funsten,Manuel Grande,Mike Gruntman,John J. Hanley,Jörg Micha Jahn,M. Jenkins,M. Lampton,M. Marckwordt,David J. McComas,Toshifumi Mukai,G. Penegor,S. Pope,S. M. Ritzau,Mark L. Schattenburg,Earl Scime,Ruth M. Skoug,W. Spurgeon,T. Stecklein,S. A. Storms,C. Urdiales,Phil Valek,J.T.M. van Beek,S. Weidner,M. Wüest,M.K. Young,C. Zinsmeyer +35 more
TL;DR: The Medium Energy Neutral Atom (MENA) imager was developed in response to the Imaging from the Magnetopause to the Aurora for Global Exploration (IMAGE) requirement to produce images of ENAs in the energy range from 1 to 30 keV as mentioned in this paper.
Book ChapterDOI
The Solar Energetic Particle Ionic Charge Analyzer (SEPICA) and the Data Processing Unit (S3DPU) for SWICS, SWIMS and SEPICA
Eberhard Möbius,L. M. Kistler,Mark A. Popecki,K. N. Crocker,M. Granoff,S. Turco,A. Anderson,P. Demain,J. Distelbrink,I. Dors,P. Dunphy,S. Ellis,J. A. Gaidos,J. Googins,R. Hayes,G. Humphrey,H. Kästle,J. Lavasseur,Eric J. Lund,R. Miller,E. Sartori,M. Shappirio,Susan Taylor,P. Vachon,M. Vosbury,V. Ye,D. Hovestadt,Berndt Klecker,H. Arbinger,E. Kunneth,Elmar Pfeffermann,E. Seidenschwang,Fritz Gliem,K.-U. Reiche,K. Stöckner,W. Wiewesiek,A. Harasim,J. Schimpfle,S. Battell,J. P. Cravens,G. Murphy +40 more
TL;DR: SEPICA as mentioned in this paper is the main instrument on the Advanced Composition Explorer (ACE) to determine the ionic charge states of solar and interplanetary energetic particles in the energy range from ≈02 MeV nucl-1 to ≈5 MeV charge-1.
Journal ArticleDOI
Plasma Experiment for Planetary Exploration (PEPE)
D. T. Young,Jane E. Nordholt,James L. Burch,David J. McComas,David J. McComas,R. P. Bowman,R. A. Abeyta,J. F. Alexander,J. R. Baldonado,P. Barker,R. K. Black,T. L. Booker,P. J. Casey,L. Cope,F. J. Crary,J. P. Cravens,Herbert O. Funsten,Raymond Goldstein,Raymond Goldstein,D. R. Guerrero,S. F. Hahn,Jennifer Hanley,B. P. Henneke,E. F. Horton,David J. Lawrence,K. McCabe,Daniel B. Reisenfeld,Daniel B. Reisenfeld,R. P. Salazar,M. Shappirio,M. Shappirio,S. A. Storms,C. Urdiales,J. H. Waite +33 more
TL;DR: The Plasma Experiment for Planetary Exploration (PEPE) as discussed by the authors is a single, low-resource instrument that uses an electrostatically swept field-of-view and a linear electric field time of flight mass spectrometer.