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.
Papers
More filters
Journal ArticleDOI
Interplanetary mesoscale observatory (InterMeso): A mission to untangle dynamic mesoscale structures throughout the heliosphere
Robert Allen,Evan Smith,J. Anderson,Joseph E. Borovsky,George C. Ho,Lan Jian,Säm Krucker,Susan T. Lepri,Gang Li,Stefano Livi,Noé Lugaz,David M. Malaspina,Bennett A. Maruca,P. Mostafavi,Jim M. Raines,Daniel Verscharen,Juliana Vievering,Sarah K. Vines,Phyllis Whittlesey,L. Wilson III,Robert F. Wimmer-Schweingruber +20 more
TL;DR: The Interplanetary Mesoscale Observatory (InterMeso) as mentioned in this paper uses a multi-point approach using four identical spacecraft in Earth-trailing orbits near 1 au.
Proceedings ArticleDOI
Strofio: A novel neutral mass spectrograph for sampling Mercury's exosphere
R. S. Gurnee,Stefano Livi,Mark Phillips,M. I. Desai,John Hayes,George C. Ho,Ramsey Hourani,S. E. Jaskulek,Juergen Scheer +8 more
TL;DR: Strofio as discussed by the authors is a scientific investigation to sample in-situ the neutral atoms in Mercury's exosphere, based on a novel mass spectrograph that determines the particle mass-per-charge (m/q) by a time-of-flight (TOF) technique.
Proceedings ArticleDOI
Observations of Particle Acceleration at Interplanetary Shocks
TL;DR: In this article, a study of in-situ interplanetary shocks and particle distributions in their vicinity provides the only meaningful way to test our theoretical understanding of shock acceleration, and the results show that more than half of these shocks produced signatures (so called energetic storm particle (ESP) events) in the low energy ion intensities.
Proceedings ArticleDOI
Propagation of impulsive solar energetic particle events
TL;DR: In this article, the authors examined the onset and ion's path-length for an impulsive solar energetic particle (SEP) in May 2000, by assuming zero degree pitch-angle scattering, and compared that with the nominal Parker spiral length.
The X-Ray Spectrometer for Mercury MESSENGER
R. D. Starr,George C. Ho,C. E. Schlemm,Robert E. Gold,John O. Goldsten,William V. Boynton,Jacob I. Trombka +6 more
TL;DR: The MESSENGER (Mercury Surface, Space Environment, Geochemistry, and Ranging) is a Discovery mission that has been designed to fly by and orbit Mercury.