The Galileo Probe Mass Spectrometer measurements in the atmosphere of Jupiter give D/H = (2.6 ± 0.7) × 10-5 3He/4He = (1.66 ± 0.05) × 10-4Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/43784/1/11214_2004_Article_184084.pd
A feature was detected at the expected wavelength for the HD R5(0) line in Jupiter's and Uranus' atm...
Abundances of hydrogen and helium isotopes in Jupiter and other giant planets can answer important q...
International audienceThe sun and giant planets are generally thought to have the same helium abunda...
During the past year, the Principal Investigator's research carried out under this contract has focu...
The mass spectrometric determinations of the isotopic composition of helium in the solar wind obtain...
We present new measurements of the deuterium abundance on Jupiter and Saturn, showing evidence that ...
The presence of excess 3He, which cannot result from air contamination, is strong evidence that indi...
$^{1}$J. T. Trauger, F. L. Roesler, N. P. Carleton, and W. A. Traub, Astrophys. J. 184, L137 (1973)....
Observations with the Short Wavelength Spectrometer (SWS) onboard the Infrared Space Observatory (IS...
Our study accomplished the first analysis of Galileo’s low/mid latitude H Lyman-α data, which contai...
We report the first direct measurement of the helium isotope ratio, 3He/4He, outside of the Local In...
The Galileo Probe Mass Spectrometer (GPMS) is a Probe instrument designed to measure the chemical an...
Abstract. The mass spectrometric determinations of the isotopic composition of helium in the solar w...
Observations with the Short Wavelength Spectrometer (SWS) onboard the Infrared Space Observatory (IS...
The Galileo Probe entered the atmosphere of Jupiter on December 7, 1995. Measurements of the chemica...
A feature was detected at the expected wavelength for the HD R5(0) line in Jupiter's and Uranus' atm...
Abundances of hydrogen and helium isotopes in Jupiter and other giant planets can answer important q...
International audienceThe sun and giant planets are generally thought to have the same helium abunda...
During the past year, the Principal Investigator's research carried out under this contract has focu...
The mass spectrometric determinations of the isotopic composition of helium in the solar wind obtain...
We present new measurements of the deuterium abundance on Jupiter and Saturn, showing evidence that ...
The presence of excess 3He, which cannot result from air contamination, is strong evidence that indi...
$^{1}$J. T. Trauger, F. L. Roesler, N. P. Carleton, and W. A. Traub, Astrophys. J. 184, L137 (1973)....
Observations with the Short Wavelength Spectrometer (SWS) onboard the Infrared Space Observatory (IS...
Our study accomplished the first analysis of Galileo’s low/mid latitude H Lyman-α data, which contai...
We report the first direct measurement of the helium isotope ratio, 3He/4He, outside of the Local In...
The Galileo Probe Mass Spectrometer (GPMS) is a Probe instrument designed to measure the chemical an...
Abstract. The mass spectrometric determinations of the isotopic composition of helium in the solar w...
Observations with the Short Wavelength Spectrometer (SWS) onboard the Infrared Space Observatory (IS...
The Galileo Probe entered the atmosphere of Jupiter on December 7, 1995. Measurements of the chemica...
A feature was detected at the expected wavelength for the HD R5(0) line in Jupiter's and Uranus' atm...
Abundances of hydrogen and helium isotopes in Jupiter and other giant planets can answer important q...
International audienceThe sun and giant planets are generally thought to have the same helium abunda...