Add to ORKGWe present here the IMAX^3He/He^4 ratios between 0.2 and 3.6 GeV /nucleon corrected to the top of the atmosphere, and a preliminary comparison with previous data. and the predictions of a standard 'Leaky Box' model of CR transport in the galaxy. We find no evidence of an excess of ^3He over that predicted by the model, in the energy range studied
5 pages, 4 figures; matches the published versionInternational audienceRecent data on Galactic cosmi...
The 3He/4He and D/p flux ratios in cosmic rays (CR) are two of the most valuable tools for understan...
One of the tests of nucleosynthesis theory is the 3He abundance in the Galaxy. 3He+ is observed thro...
We present here the IMAX^3He/He^4 ratios between 0.2 and 3.6 GeV /nucleon corrected to the top of t...
The rare isotopes ^2H and ^3He in cosmic rays are believed to originate mainly from the interaction ...
We report the first direct measurement of the helium isotope ratio, 3He/4He, outside of the Local In...
The abundances of cosmic-ray helium isotopes between 0.2 and 3.7 GeV nucleon^(-1) were measured by t...
The abundances of cosmic-ray helium isotopes between 0.2 and 3.7 GeV nucleon^(-1) were measured by ...
International audienceWe report the first direct measurement of the helium isotope ratio, $^{3}$He/$...
We have reexamined the implications of a recent measurement of cosmic-ray ^3He at ~6 GeV per nucleon...
We summarize the current status of the so-called "He-3 problem", and we discuss successes and failur...
The rare isotopes ^(2)H and ^(3)He in cosmic rays are believed to originate mainly from the interact...
International audienceThe helium isotope composition of air might have changed since the industrial ...
The Superconducting Magnet Instrument for Light Isotopes (SMILI) flew for 19 hours on 1989 September...
The Caltech Electron/Isotope Spectrometer on IMP-7 has been used to identify the isotopes ^2H and ^...
5 pages, 4 figures; matches the published versionInternational audienceRecent data on Galactic cosmi...
The 3He/4He and D/p flux ratios in cosmic rays (CR) are two of the most valuable tools for understan...
One of the tests of nucleosynthesis theory is the 3He abundance in the Galaxy. 3He+ is observed thro...
We present here the IMAX^3He/He^4 ratios between 0.2 and 3.6 GeV /nucleon corrected to the top of t...
The rare isotopes ^2H and ^3He in cosmic rays are believed to originate mainly from the interaction ...
We report the first direct measurement of the helium isotope ratio, 3He/4He, outside of the Local In...
The abundances of cosmic-ray helium isotopes between 0.2 and 3.7 GeV nucleon^(-1) were measured by t...
The abundances of cosmic-ray helium isotopes between 0.2 and 3.7 GeV nucleon^(-1) were measured by ...
International audienceWe report the first direct measurement of the helium isotope ratio, $^{3}$He/$...
We have reexamined the implications of a recent measurement of cosmic-ray ^3He at ~6 GeV per nucleon...
We summarize the current status of the so-called "He-3 problem", and we discuss successes and failur...
The rare isotopes ^(2)H and ^(3)He in cosmic rays are believed to originate mainly from the interact...
International audienceThe helium isotope composition of air might have changed since the industrial ...
The Superconducting Magnet Instrument for Light Isotopes (SMILI) flew for 19 hours on 1989 September...
The Caltech Electron/Isotope Spectrometer on IMP-7 has been used to identify the isotopes ^2H and ^...
5 pages, 4 figures; matches the published versionInternational audienceRecent data on Galactic cosmi...
The 3He/4He and D/p flux ratios in cosmic rays (CR) are two of the most valuable tools for understan...
One of the tests of nucleosynthesis theory is the 3He abundance in the Galaxy. 3He+ is observed thro...