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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Proceedings ArticleDOI
ACE Observations of Energetic Particles Associated with Transient Interplanetary Shocks
TL;DR: A survey of the effects of interplanetary shocks on energetic >47 keV ions and >38 keV electrons as observed by the ACE spacecraft from September 1997 to December 2001 is presented in this article.
Journal ArticleDOI
MESSENGER detection of electron-induced X-ray fluorescence from Mercury's surface
R. D. Starr,David Schriver,Larry R. Nittler,Shoshana Z. Weider,Paul K. Byrne,George C. Ho,Edgar A. Rhodes,C. E. Schlemm,Sean C. Solomon,Sean C. Solomon,Pavel M. Trávníček +10 more
TL;DR: The X-Ray Spectrometer (XRS) on the MESSENGER spacecraft measured elemental abundances on the surface of Mercury by detecting fluorescent X-ray emissions induced on the planet's surface by the incident solar Xray flux as mentioned in this paper.
Journal ArticleDOI
MESSENGER observations of Mercury's magnetosphere during northward IMF
James A. Slavin,Brian J. Anderson,Thomas H. Zurbuchen,Daniel N. Baker,Stamatios M. Krimigis,Stamatios M. Krimigis,Mario H. Acuña,Mehdi Benna,Scott A. Boardsen,George Gloeckler,George Gloeckler,Robert E. Gold,George C. Ho,Haje Korth,Ralph L. McNutt,Jim M. Raines,Menelaos Sarantos,David Schriver,Sean C. Solomon,Pavel Trávníček +19 more
TL;DR: In this article, MESSENGER's January 14, 2008, flyby of Mercury has provided new observations of the planet's magnetosphere for northward interplanetary magnetic field (IMF).
Journal ArticleDOI
Effects of wave superposition on the polarization of electromagnetic ion cyclotron waves
TL;DR: In this paper, a detailed comparison between the observed polarization properties of electromagnetic ion cyclotron (EMIC) waves and those predicted by theory was made using data from the Active Magnetospheric Particle Tracer Explorers/charge composition Explorer spacecraft.
Journal ArticleDOI
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 to observe a high-temperature, multispecies population of energetic particles, and velocity dispersions, anisotropies, and compositional variation seen in the deep-tail (≳ 500 R J) with a ∼3-day periodicity are similar to variations seen closer to Jupiter in Galileo data.