Add to ORKGThe energy dependence of the mean escape length of cosmic rays from the galaxy in the light of recent measurements of cosmic ray abundances from the Danish-French experiment on HEAO-3 is re-examined. The energy dependence is found to be steeper than previously thought
The Galactic cosmic ray spectrum is a remarkably straight power law. Our current understanding is th...
The small flotilla of spacecraft: Pioneers 10 and 11 and Voyagers 1 and 2 (V1 and V2) that have trav...
At energies below ~300 MeV/nuc our knowledge of cosmic-ray spectra outside the heliosphere is obscur...
The variation of the 5 to 500 MeV/nuc cosmic ray helium component was studied between 1 and 9 A.U. u...
The study of systematic trends in elemental abundances is important for unfolding the nuclear and/or...
The origin and propagation of cosmic rays in terms of conventional and supplementary newer assumptio...
Galactic cosmic ray (GCR) secondary/primary ratios such as B/C and (Sc+Ti+V)/Fe are commonly used to...
Acceleration and propagation of solar cosmic rays as deduced from relative abundance of protons to h...
Recent accurate measurements of the cosmic-ray intensity ratio ^(51)V/^(51)Cr below 1 GeV nucleon^(-...
Galactic cosmic ray (GCR) secondary/primary ratios such as B/C and (Sc+Ti+V)/Fe are commonly used to...
Voyager 1 has now been beyond the heliopause for over 5 years since its seminal crossing of this bou...
The HEAO-3 Heavy Nuclei Experiment has measured abundances of elements from Ar-18 to U-92 in the cos...
In a previous study (Maurin et al., 2001), we explored the set of parameters describing diffusive pr...
The relative abundance of nuclear species measured in cosmic rays at Earth has often been interprete...
We present energy spectra of anomalous cosmic ray hydrogen, helium, and oxygen derived from data co...
The Galactic cosmic ray spectrum is a remarkably straight power law. Our current understanding is th...
The small flotilla of spacecraft: Pioneers 10 and 11 and Voyagers 1 and 2 (V1 and V2) that have trav...
At energies below ~300 MeV/nuc our knowledge of cosmic-ray spectra outside the heliosphere is obscur...
The variation of the 5 to 500 MeV/nuc cosmic ray helium component was studied between 1 and 9 A.U. u...
The study of systematic trends in elemental abundances is important for unfolding the nuclear and/or...
The origin and propagation of cosmic rays in terms of conventional and supplementary newer assumptio...
Galactic cosmic ray (GCR) secondary/primary ratios such as B/C and (Sc+Ti+V)/Fe are commonly used to...
Acceleration and propagation of solar cosmic rays as deduced from relative abundance of protons to h...
Recent accurate measurements of the cosmic-ray intensity ratio ^(51)V/^(51)Cr below 1 GeV nucleon^(-...
Galactic cosmic ray (GCR) secondary/primary ratios such as B/C and (Sc+Ti+V)/Fe are commonly used to...
Voyager 1 has now been beyond the heliopause for over 5 years since its seminal crossing of this bou...
The HEAO-3 Heavy Nuclei Experiment has measured abundances of elements from Ar-18 to U-92 in the cos...
In a previous study (Maurin et al., 2001), we explored the set of parameters describing diffusive pr...
The relative abundance of nuclear species measured in cosmic rays at Earth has often been interprete...
We present energy spectra of anomalous cosmic ray hydrogen, helium, and oxygen derived from data co...
The Galactic cosmic ray spectrum is a remarkably straight power law. Our current understanding is th...
The small flotilla of spacecraft: Pioneers 10 and 11 and Voyagers 1 and 2 (V1 and V2) that have trav...
At energies below ~300 MeV/nuc our knowledge of cosmic-ray spectra outside the heliosphere is obscur...