G
George C. Ho
Researcher at Johns Hopkins University Applied Physics Laboratory
Publications - 164
Citations - 4886
George C. Ho is an academic researcher from Johns Hopkins University Applied Physics Laboratory. The author has contributed to research in topics: Solar wind & Magnetosphere. The author has an hindex of 33, co-authored 135 publications receiving 3958 citations. Previous affiliations of George C. Ho include Johns Hopkins University & University of Maryland, College Park.
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Journal ArticleDOI
Comprehensive survey of energetic electron events in Mercury's magnetosphere with data from the MESSENGER Gamma-Ray and Neutron Spectrometer
David J. Lawrence,Brian J. Anderson,Daniel N. Baker,William C. Feldman,George C. Ho,Haje Korth,Ralph L. McNutt,Patrick N. Peplowski,Sean C. Solomon,Sean C. Solomon,R. D. Starr,Jon Vandegriff,Reka M. Winslow,Reka M. Winslow +13 more
TL;DR: In this paper, the authors used the MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) Gamma-Ray and Neutron Spectrometer data to detect and characterize energetic electron (EE) events in Mercury's magnetosphere.
Journal ArticleDOI
Quasi‐trapped ion and electron populations at Mercury
David Schriver,Pavel M. Trávníček,Pavel M. Trávníček,Brian J. Anderson,Maha Ashour-Abdalla,Daniel N. Baker,Mehda Benna,Scott A. Boardsen,Robert E. Gold,Petr Hellinger,George C. Ho,Haje Korth,Stamatios M. Krimigis,Stamatios M. Krimigis,Ralph L. McNutt,Jim M. Raines,Robert L. Richard,James A. Slavin,Sean C. Solomon,R. D. Starr,Thomas H. Zurbuchen +20 more
TL;DR: In this paper, an equatorially centered distribution of plasma at 1.4 RM radial distance (where RMis Mercury's radius) around a substantial portion of the planet in local time from morning through night and into the afternoon sector was observed.
Energetic Particles in the Jovian Magnetotail
Ralph L. McNutt,Dennis Haggerty,Matthew E. Hill,Stamatios M. Krimigis,Stamatios M. Krimigis,Stefano Livi,George C. Ho,R. S. Gurnee,Barry Mauk,D. G. Mitchell,E. C. Roelof,David J. McComas,Fran Bagenal,H. A. Elliott,L. E. Brown,M. Kusterer,Jon Vandegriff,S. A. Stern,Harold A. Weaver,John R. Spencer,Jeffrey M. Moore +20 more
TL;DR: The New Horizons spacecraft traversed the length of the jovian magnetotail, observing a high-temperature, multispecies population of energetic particles, suggesting plasma streaming away from the planet and injection sites in the near-tail region that could be related to magnetic reconnection events.
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Solar Wind Streams and Stream Interaction Regions Observed by the Parker Solar Probe with Corresponding Observations at 1 au
Robert Allen,David Lario,Dusan Odstrcil,George C. Ho,Lan Jian,Christina Cohen,Samuel T. Badman,Shaela I. Jones,C. N. Arge,M. L. Mays,G. M. Mason,Stuart D. Bale,John W. Bonnell,Anthony W. Case,E. R. Christian,T. Dudok de Wit,Keith Goetz,Peter Harvey,Carl J. Henney,Matthew E. Hill,Justin C. Kasper,K. E. Korreck,Davin Larson,Roberto Livi,Robert J. MacDowall,David M. Malaspina,D. J. McComas,Ralph L. McNutt,Donald G. Mitchell,Marc Pulupa,N.-E. Raouafi,Nathan A. Schwadron,Michael L. Stevens,Phyllis Whittlesey,Mark E. Wiedenbeck +34 more
TL;DR: In this paper, the Parker Solar Probe (PSP) observed several fast solar wind streams and stream interaction regions (SIRs) during its first orbit (2018 September-2019 January) during this time, several recurring SIRs were also seen at 1 au at both L1 (Advanced Composition Explorer) and Wind) and the location of the Solar Terrestrial Relations Observatory-Ahead (STEREO-A).
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MESSENGER and Venus Express observations of the solar wind interaction with Venus
James A. Slavin,Mario H. Acuña,Brian J. Anderson,Stas Barabash,Mehdi Benna,Scott A. Boardsen,Markus Fraenz,George Gloeckler,Robert E. Gold,George C. Ho,Haje Korth,Stamatios M. Krimigis,Ralph L. McNutt,Jim M. Raines,Menelaos Sarantos,Sean C. Solomon,Tielong Zhang,Thomas H. Zurbuchen +17 more
TL;DR: Stavin et al. as mentioned in this paper presented MESSENGER observations of new features of the Venus - solar wind interaction including hot flow anomalies upstream of the bow shock, a flux rope in the near-tail and a two-point determination of the timescale for magnetic flux transport through this induced magnetosphere.