A definitive study of the elemental abundances of nuclei over the charge range of 20 ≤ Z ≤ 100 requires a satellite mission capable of obtaining high statistics and excellent charge resolution over the full charge range. Such a mission, utilizing an electronic instrument which is an evolution of the HEA0-3 Heavy Nuclei Experiment, is described here
The HEAO-3 Heavy Nuclei Experiment has measured elemental abundances of ultraheavy cosmic rays near...
The HEAO-3 Heavy Nuclei Experiment has measured elemental abundances of ultraheavy cosmic rays near...
An apparatus has been designed and is being fabricated to study the charge composition, fluxes, and ...
A definitive study of the elemental abundances of nuclei over the charge range of 20 ≤ Z ≤ 100 requi...
A definitive study of the elemental abundances of nuclei over the charge range of 20 ≤ Z ≤ 100 requi...
The third High Energy Astronomical Observatory, HEAO-3 was launched on the 20th Sept., 1979 into a 4...
The third High Energy Astronomical Observatory, HEAO-3 was launched on the 20th Sept., 1979 into a 4...
Measurements of the elemental abundances of galactic cosmic ray nuclei with charge 26≤z≤92 can provi...
Measurements of the elemental abundances of galactic cosmic ray nuclei with charge 26≤z≤92 can provi...
Journal ArticleThe accurate determination of the elemental composition of cosmic rays at high energi...
The Final Report on the continuing analysis of data from the Heavy Nuclei Experiment (HNE), flown on...
A group collaboration was made in the development of the Bristol University Gas Spectrometer number ...
A wealth of information regarding cosmic ray synthesis and propagation is contained in the ultra‐hea...
The Ultra Heavy Cosmic Ray Experiment (UHCRE) is based on a modular array of 192 side-viewing solid ...
The composition and energy spectra of cosmic rays above 1.6 nJ (10 GeV) on balloons and ultimately o...
The HEAO-3 Heavy Nuclei Experiment has measured elemental abundances of ultraheavy cosmic rays near...
The HEAO-3 Heavy Nuclei Experiment has measured elemental abundances of ultraheavy cosmic rays near...
An apparatus has been designed and is being fabricated to study the charge composition, fluxes, and ...
A definitive study of the elemental abundances of nuclei over the charge range of 20 ≤ Z ≤ 100 requi...
A definitive study of the elemental abundances of nuclei over the charge range of 20 ≤ Z ≤ 100 requi...
The third High Energy Astronomical Observatory, HEAO-3 was launched on the 20th Sept., 1979 into a 4...
The third High Energy Astronomical Observatory, HEAO-3 was launched on the 20th Sept., 1979 into a 4...
Measurements of the elemental abundances of galactic cosmic ray nuclei with charge 26≤z≤92 can provi...
Measurements of the elemental abundances of galactic cosmic ray nuclei with charge 26≤z≤92 can provi...
Journal ArticleThe accurate determination of the elemental composition of cosmic rays at high energi...
The Final Report on the continuing analysis of data from the Heavy Nuclei Experiment (HNE), flown on...
A group collaboration was made in the development of the Bristol University Gas Spectrometer number ...
A wealth of information regarding cosmic ray synthesis and propagation is contained in the ultra‐hea...
The Ultra Heavy Cosmic Ray Experiment (UHCRE) is based on a modular array of 192 side-viewing solid ...
The composition and energy spectra of cosmic rays above 1.6 nJ (10 GeV) on balloons and ultimately o...
The HEAO-3 Heavy Nuclei Experiment has measured elemental abundances of ultraheavy cosmic rays near...
The HEAO-3 Heavy Nuclei Experiment has measured elemental abundances of ultraheavy cosmic rays near...
An apparatus has been designed and is being fabricated to study the charge composition, fluxes, and ...