Zobrazeno 1 - 10
of 52
pro vyhledávání: '"Charles W. Hord"'
Publikováno v:
Journal of Geophysical Research: Planets. 104:14169-14178
We report on Ultraviolet Spectrometer observations of Ganymede from four orbits of the Galileo primary mission. During 12 observation sequences, regions on Ganymede's leading, trailing, and anti-Jovian hemispheres were observed at several latitudes a
Publikováno v:
Journal of Geophysical Research: Planets. 104:11817-11826
The Galileo ultraviolet spectrometer has observed Jupiter's volcanically active moon Io in the 2100–3200 A wavelength range at 13.7 A resolution. We find that both sulfur dioxide frost on the surface and sulfur dioxide gas in Io's atmosphere are de
Publikováno v:
Icarus. 135:79-94
The Galileo ultraviolet spectrometer has measured the first-ever disk-resolved spectral ultraviolet albedos of regions on Europa's trailing and antijovian hemispheres at spatial resolutions approaching 55 km. We find that the ultraviolet albedo (2400
Autor:
Wayne R. Pryor, G. K. James, Deborah A. Miller, A. Ian F. Stewart, Stuart K. Stephens, Charles W. Hord, Amanda R. Hendrix, Donald E. Shemansky, W. Kent Tobiska, Joseph M. Ajello, Robert A. West, William E. McClintock, Karen E. Simmons
Publikováno v:
Journal of Geophysical Research: Planets. 103:20149-20158
In 1996 and 1997 the Galileo Ultraviolet Spectrometer (UVS) obtained the first measurements of Jupiter's nightside midultraviolet (MUV) polar auroral spectrum from 1620 to 3231 A at 13 A resolution. The reduced polar spectra, after removal of off-axi
Autor:
Stuart K. Stephens, Ian Stewart, Charles A. Barth, Karen E. Simmons, Charles W. Hord, Wayne R. Pryor, Deborah A. Miller, William E. McClintock, Joseph M. Ajello, John Clarke, Jeremy Gebben, Bill R. Sandel, K. Tobiska, Donald E. Shemansky
Publikováno v:
Journal of Geophysical Research: Planets. 103:20125-20148
In 1996 during the first four orbits of the satellite tour the Galileo ultraviolet spectrometer (UVS) (11304320 A) and extreme ultraviolet spectrometer (EUVS) (540-1280 A) performed near-simultaneous observations of the Jupiter aurora in both the nor
Autor:
K. L. Naviaux, Charles A. Barth, A. I. F. Stewart, Joseph M. Ajello, Charles W. Hord, Karen E. Simmons, J. J. Aiello, William E. McClintock, Wayne R. Pryor
Publikováno v:
Geophysical Research Letters. 24:2147-2150
Atomic hydrogen Lyman alpha radiation (121.6 nm) has been measured in emission from the atmosphere of Ganymede with the Galileo ultraviolet spectrometer. An exospheric model with the following parameters has been fit to the observational data: atomic
Autor:
William E. McClintock, J. J. Gebben, Charles W. Hord, Charles A. Barth, Oran R. White, W. K. Tobiska, Wayne R. Pryor, K. L. Naviaux, S. Lineaweaver, S. J. Edberg, Karen E. Simmons, Bill R. Sandel, A. I. F. Stewart, Joseph M. Ajello
Publikováno v:
Geophysical Research Letters. 23:1893-1896
Observations of interplanetary Lyman-α obtained by the Galileo Extreme Ultraviolet Spectrometer (EUVS) experiment near solar maximum in 1990 show a distinct migration in the upwind brightness maximum from 36±5°N to 6±5°N ecliptic latitude over a
Autor:
J. J. Gebben, W. K. Tobiska, Wayne R. Pryor, K. L. Naviaux, Joseph M. Ajello, Charles A. Barth, Larry W. Esposito, S. J. Edberg, Robert A. West, A. I. F. Stewart, Karen E. Simmons, Charles W. Hord, William E. McClintock
Publikováno v:
Geophysical Research Letters. 22:1565-1568
The Galileo Ultraviolet Spectrometer (UVS) team has detected the Shoemaker-Levy 9 fragment G impact on Jupiter in data recently played back from the spacecraft tape recorder. A 20% brightening of the disc-integrated signal of Jupiter was detected at
Publikováno v:
Advances in Space Research. 13:37-40
The Galileo Ultraviolet Spectrometer Experiment (UVS) obtained a map of the celestial sphere from interplanetary Lyman-alpha (IPLA) on 13, 14 December 1990 during the Earth1 encounter. The Galileo spacecraft was near the downwind interstellar axis du
Autor:
Wayne R. Pryor, Charles W. Hord
Publikováno v:
Icarus. 91:161-172
The present investigation of the dark hazes of Jupiter, Saturn, Uranus, and Neptune on the basis of Voyager 2 UV data notes a geographic correlation between the auroral zones of Jupiter and Saturn and UV-dark polar regions. While the auroral fluxes a