8 Papers
59 Citations
J. Hui is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Jupiter & Atmosphere of Jupiter. The author has an hindex of 4, co-authored 8 publications.
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Papers
Galileo infrared observations of the Shoemaker‐Levy 9 G Impact Fireball: A Preliminary report
Robert W. Carlson,Paul R. Weissman,M. Segura,J. Hui,William D. Smythe,Torrence V. Johnson,Kevin H. Baines,Pierre Drossart,Th. Encrenaz,F. Leader +9 more
TL;DR: The Galileo spacecraft was fortuitously situated for a direct view of the impacts of the fragments of comet Shoemaker-Levy 9 in Jupiter's atmosphere, and the Near Infrared Mapping Spectrometer instrument observed several of the impact events in several discrete bands and with a temporal resolution of roughly five seconds as mentioned in this paper.
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Galileo Infrared Observations of the Shoemaker-Levy 9 G and R Fireballs and Splash
R. W. Carlson,Paul R. Weissman,J. Hui,M. Segura,W. D. Smythe,K. H. Baines,T. V. Johnson,P. Drossart,T. Encrenaz,F. Leader,R. Mehlman +10 more
- 01 Feb 1995
TL;DR: The Galileo spacecraft was positioned for a direct view of the impacts of comet Shoemaker(ka)evy 9 in Jupiter's atmosphere and measurements were recorded by the Near Infrared Mapping Spectrometer (NIMS) instrument for several of the impact events as mentioned in this paper.
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Surface Composition of the Galilean Satellites from Galileo Near Infrared Mapping Spectroscopy
Robert W. Carlson,William D. Smythe,Dennis L. Matson,R. Lopes-Gautier,J. Hui,M. Segura,Adriana C. Ocampo,Laurence A. Soderblom,Hugh H. Kieffer,Thomas B. McCord,Fraser P. Fanale,G. E. Hansen +11 more
TL;DR: The Galileo Near Infrared Mapping Spectrometer (NIMS) is currently obtaining spectral maps of Jupiter's moons to determine the composition and spatial distribution of minerals on the satellite surfaces as mentioned in this paper.
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Particle sizes of the Uranus delta ring's inner diffuse companion through comparison of RSS and PPS voyager occultation data
J. Hui,L. J. Horn,Arthur L. Lane +2 more
TL;DR: In this article, an inner diffuse companion of the Uranian delta ring was detected and found to have an average width of 12 km by comparing the widths and equivalent depths of the two sets of data, it was established that the particles making the greatest contribution to the integrated opacities of the companion are of greater than several cm sizes.
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