Search Results - "Hunten, D."
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The abundances of constituents of Titan's atmosphere from the GCMS instrument on the Huygens probe
Published in Nature (08-12-2005)“…Saturn's largest moon, Titan, remains an enigma, explored only by remote sensing from Earth, and by the Voyager and Cassini spacecraft. The most puzzling…”
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The sequestration of ethane on Titan in smog particles
Published in Nature (12-10-2006)“…Saturn's largest satellite, Titan, has a dense atmosphere of nitrogen with a few per cent of methane. At visible wavelengths its surface is hidden by dense…”
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Helium in Jupiter's atmosphere: Results from the Galileo probe Helium Interferometer Experiment
Published in Journal of Geophysical Research, Washington, DC (25-09-1998)“…On December 7, 1995, the NASA Galileo probe provided the first in situ measurements of the helium abundance in the atmosphere of Jupiter. Our Jamin…”
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4
Mars' South Polar Ar Enhancement: A Tracer for South Polar Seasonal Meridional Mixing
Published in Science (American Association for the Advancement of Science) (19-11-2004)“…The gamma ray spectrometer on the Mars Odyssey spacecraft measured an enhancement of atmospheric argon over southern high latitudes during autumn followed by…”
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The composition of the Jovian atmosphere as determined by the Galileo probe mass spectrometer
Published in Journal of Geophysical Research, Washington, DC (25-09-1998)“…The Galileo probe mass spectrometer determined the composition of the Jovian atmosphere for species with masses between 2 and 150 amu from 0.5 to 21.1 bars…”
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Mars atmospheric water vapor abundance: 1991–1999, emphasis 1998–1999
Published in Icarus (New York, N.Y. 1962) (01-10-2006)“…Our ground-based measurements of martian atmospheric water vapor, made throughout L s = 34 ° to 249°, 24 September 1998 to 23 November 1999, during Mars year…”
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The Galileo Probe Mass Spectrometer: Composition of Jupiter's Atmosphere
Published in Science (American Association for the Advancement of Science) (10-05-1996)“…The composition of the jovian atmosphere from 0.5 to 21 bars along the descent trajectory was determined by a quadrupole mass spectrometer on the Galileo…”
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The Helium Mass Fraction in Jupiter's Atmosphere
Published in Science (American Association for the Advancement of Science) (10-05-1996)“…On 7 December 1995, the NASA Galileo probe provided in situ measurements of the helium abundance in the atmosphere of Jupiter. A Jamin interferometer measured…”
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9
The Gas Chromatograph Mass Spectrometer for the Huygens Probe
Published in Space science reviews (01-01-2002)“…The Gas Chromatograph Mass Spectrometer (GCMS) on the Huygens Probe will measure the chemical composition of Titan's atmosphere from 170 km altitude (1 hPa) to…”
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Observations of Mercury's exosphere: Spatial distributions and variations of its Na component during August 8, 9 and 10, 2003
Published in Icarus (New York, N.Y. 1962) (01-12-2006)“…Following the observations of August 2002 [Barbieri, C., Verani, S., Cremonese, G., Sprague, A., Mendillo, M., Cosentino, R., Hunten, D., 2004. Planet. Space…”
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Planetary science. Clues to the Martian atmosphere
Published in Science (American Association for the Advancement of Science) (30-11-2001)Get full text
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Mercury's exosphere origins and relations to its magnetosphere and surface
Published in Planetary and space science (01-06-2007)“…Mariner 10, the only spacecraft that ever passed close to Mercury, revealed several unexpected characteristics: an intrinsic magnetosphere, the highest mean…”
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Distribution and Abundance of Sodium in Mercury's Atmosphere, 1985–1988
Published in Icarus (New York, N.Y. 1962) (01-10-1997)“…We report spectroscopic measurements of sodium in Mercury's atmosphere for the period July 1985–May 1988. Na abundance varies from <1 × 1010atoms cm−2in…”
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14
Origin and character of the lunar and mercurian atmospheres
Published in Advances in space research (01-01-1997)“…This article presents a description of the lunar and mercurian atmospheres and the outstanding, unanswered questions. In that spirit we will not repeat the…”
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Mars atmospheric water vapor abundance: 1996–1997
Published in Icarus (New York, N.Y. 1962) (01-05-2003)“…Measurements of martian atmospheric water vapor made throughout L s = 18.0°–146.4° (October 3, 1996–July 12, 1997) show changes in Mars humidity on hourly,…”
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Correction for Dust Opacity of Martian Atmospheric Water Vapor Abundances
Published in Icarus (New York, N.Y. 1962) (01-09-2000)“…A method is presented to correct for the effects of dust opacity on the derivation of water-vapor abundances from observed spectral absorption lines. We show…”
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17
Mars' South Polar Ar Enhancement: A Tracer for South Polar Seasonal Meridional Mixing
Published in Science (American Association for the Advancement of Science) (19-11-2004)“…The gamma ray spectrometer on the Mars Odyssey spacecraft measured an enhancement of atmospheric argon over southern high latitudes during autumn followed by…”
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18
The Leonid Meteor Shower and the Lunar Sodium Atmosphere
Published in Icarus (New York, N.Y. 1962) (01-12-1998)“…Observations of lunar sodium were made on November 16–18, 1997, at Asiago and Mount Lemmon Observatories. A small enhancement was observed, and we suggest that…”
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Water Vapor Abundances over Mars North High Latitude Regions: 1996–1999
Published in Icarus (New York, N.Y. 1962) (01-11-2001)“…We present column abundances of water vapor in Mars' atmosphere over high north latitudes for L s 46°–146° during 1996–1997 and L s 34°–180° during 1998–1999…”
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Diurnal variation of sodium and potassium at Mercury
Published in Meteoritics & planetary science (01-09-2002)“…— A summary is given of our published observations showing a large (3 to 4) morning/afternoon ratio of the abundances of sodium and potassium. The proposed…”
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