Zobrazeno 1 - 10
of 41
pro vyhledávání: '"W. H. Smyth"'
Longitudinal modulation of the brightness of Io's auroral footprint emission: Comparison with models
Autor:
Fran Bagenal, Suwicha Wannawichian, Jonathan D. Nichols, W. H. Smyth, John Clarke, C. A. Peterson
Publikováno v:
Journal of Geophysical Research: Space Physics. 118:3336-3345
[1] The auroral emission close to the foot of Io's magnetic flux tube has been known for over a decade to be one of the key parameters characterizing the electrodynamic interaction between the satellite and Jupiter's magnetosphere. Ten years of obser
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3c6651163aa7912e1ff9054d14145863
https://doi.org/10.1002/jgra.50346
https://doi.org/10.1002/jgra.50346
Autor:
Michael J. S. Belton, K. Rages, William B. Hubbard, Paul Geissler, Torrence V. Johnson, A. J. Dessler, Alfred S. McEwen, Wing-Huen Ip, W. H. Smyth, Andrew P. Ingersoll
Publikováno v:
Journal of Geophysical Research: Space Physics. 106:26137-26146
Clear-filter imaging of Io during the Galileo nominal and extended missions recorded diffuse auroral emissions in 16 distinct observations taken during 14 separate eclipses over a two year period. These images show that the morphology and time variab
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7810d6549dc7dbc95325a958488fb688
https://doi.org/10.1029/2000ja002511
https://doi.org/10.1029/2000ja002511
Autor:
W. H. Smyth, M. L. Marconi
Publikováno v:
Journal of Geophysical Research: Space Physics. 105:7783-7792
From modeling analysis of two different ground-based observations for Io's neutral oxygen cloud in [O I] 6300 A emission, new exobase atomic oxygen source rates produced by the composite effects of ion sputtering (represented by an incomplete collisi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::605bd68f4c62a20ddea02349a4908ce2
https://doi.org/10.1029/1999ja000308
https://doi.org/10.1029/1999ja000308
Autor:
Ronald J. Oliversen, Kurt D. Retherford, R. C. Woodward, W. H. Smyth, H. W. Moos, Darrell F. Strobel, Fred L. Roesler, M. A. McGrath, P. D. Feldman, Frank Scherb
Publikováno v:
Science. 283:353-357
Well-resolved far-ultraviolet spectroscopic images of O i , S i , and previously undetected H i Lyman-α emission from Io were obtained with the Hubble space telescope imaging spectrograph (STIS). Detected O i and S i lines (1250 to 1500 angstroms) h
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d06c6a46c692542e25efcdd2c93f728f
https://doi.org/10.1126/science.283.5400.353
https://doi.org/10.1126/science.283.5400.353
Publikováno v:
Journal of Geophysical Research: Planets. 103:19935-19946
The Io plasma torus apparently has a much longer lifetime than anticipated on the basis of simple theoretical stability analyses. This quandary is particularly evident at the outer edge of the torus, the plasma ramp, where the steep radial gradient i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::43e824c79b8f04c7b7438db031c6570b
https://doi.org/10.1029/98je00538
https://doi.org/10.1029/98je00538
Autor:
Girolamo Benzoni, W. H. Smyth
Publikováno v:
History of the New World: Shewing His Travels in America, from A.D. 1541 to 1556: with Some Particulars of the Island of Canary
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::00d2d4b8d6b4efac479e69bda4450235
https://doi.org/10.1017/cbo9780511694615.001
https://doi.org/10.1017/cbo9780511694615.001
Autor:
Andrew P. Ingersoll, Torrence V. Johnson, Alfred S. McEwen, Michael J. S. Belton, Paul Geissler, Wing-Huen Ip, W. H. Smyth
Publikováno v:
Science (New York, N.Y.). 285(5429)
The Galileo spacecraft has detected diffuse optical emissions from Io in high-resolution images acquired while the satellite was eclipsed by Jupiter. Three distinct components make up Io's visible emissions. Bright blue glows of more than 300 kiloray
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5a546e796911c53bc10be7a0eb0ff0c0
https://pubmed.ncbi.nlm.nih.gov/10436151
https://pubmed.ncbi.nlm.nih.gov/10436151
Autor:
Alain Roux, Fran Bagenal, Christopher T. Russell, C. Polanskey, W. H. Ip, Scott Bolton, W. H. Smyth, Andrew F. Cheng
Publikováno v:
Eos, Transactions American Geophysical Union. 78:93
When the Galileo orbiter passed within 1000 km of Io on December 7, 1995, the data collected were every bit as exciting as the Galileo team had expected, given the unique interaction between Io and the Jovian magnetosphere. The spacecraft detected in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::48d89423cfb85ac4b85bffad3c84aa52
https://doi.org/10.1029/97eo00059
https://doi.org/10.1029/97eo00059
Autor:
Frank Scherb, W. H. Smyth
Publikováno v:
Journal of Geophysical Research. 98:18729
Observations of (O I) 6300-A emission near Io have been obtained in 1990, 1991, and 1992 by the National Solar Observatory staff using the solar-stellar spectrography on the McMath-Pierce telescope at Kitt Peak. High-resolution spectra with a resolvi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2fc9f7c05f435534afd5e1d819108a4a
https://doi.org/10.1029/93je00539
https://doi.org/10.1029/93je00539