The importance of Lead and Uranium group abundances in cosmic rays is discussed in understanding their evolution and propagation. The electronic detectors can provide good charge resolution but poor data statistics. The plastic detectors can provide somewhat better statistics but charge resolution deteriorates. The extraterrestrial crystals can provide good statistics but with poor charge resolution. Recent studies of extraterrestrial crystals regarding their calibration to accelerated uranium ion beam and track etch kinetics are discussed. It is hoped that a charge resolution of two charge units can be achieved provided an additional parameter is taken into account. The prospects to study abundances of Lead group, Uranium group and superhe...
A passive, large‐area experiment for the detection of cosmic ray actinides on the lunar surface is d...
The relative abundances of elements in the charge ranges of 75 ≤ Z ≤ 79 (platinum) and 80 ≤ Z ≤ 83 (...
The suggestions that the source abundances of cosmic ray nuclei heavier then Fe differ significantly...
This paper reports an observation of the abundances of cosmic-ray lead and platinum-group nuclei us...
Experiments were carried out on tracks of high energy U ions in olivine, a common meteoritic mineral...
Observations of the abundances of elements of charge 62 or Z or = 73 in the cosmic radiation from th...
A wealth of information regarding cosmic ray synthesis and propagation is contained in the ultra‐hea...
ABSTRACT The DIAS-ESTEC Ultra Heavy Cosmic Ray Experiment (UHCRE) on the Long Duration Exposure Faci...
Analysis of a new, higher resolution data set from the Heavy Nuclei Experiment on the HEA0-3 spacec...
The Ultra Heavy Cosmic Ray Experiment (UHCRE) is based on a modular array of 192 side-viewing solid ...
The HEAO 3 detector of heavy cosmic-ray nuclei has observed one possible actinide nucleus and some ...
We report here an analysis that, for the first time, systematically normalizes the data from the HEA...
The HEAO-3 Heavy Nuclei Experiment has measured elemental abundances of ultraheavy cosmic rays near...
Data extraction and analysis of the LDEF Ultra Heavy Cosmic Ray Experiment is continuing. Almost twi...
Abundances relative to _(96)Fe have been derived for elements with charge, 2, in the range 32≤z≤40. ...
A passive, large‐area experiment for the detection of cosmic ray actinides on the lunar surface is d...
The relative abundances of elements in the charge ranges of 75 ≤ Z ≤ 79 (platinum) and 80 ≤ Z ≤ 83 (...
The suggestions that the source abundances of cosmic ray nuclei heavier then Fe differ significantly...
This paper reports an observation of the abundances of cosmic-ray lead and platinum-group nuclei us...
Experiments were carried out on tracks of high energy U ions in olivine, a common meteoritic mineral...
Observations of the abundances of elements of charge 62 or Z or = 73 in the cosmic radiation from th...
A wealth of information regarding cosmic ray synthesis and propagation is contained in the ultra‐hea...
ABSTRACT The DIAS-ESTEC Ultra Heavy Cosmic Ray Experiment (UHCRE) on the Long Duration Exposure Faci...
Analysis of a new, higher resolution data set from the Heavy Nuclei Experiment on the HEA0-3 spacec...
The Ultra Heavy Cosmic Ray Experiment (UHCRE) is based on a modular array of 192 side-viewing solid ...
The HEAO 3 detector of heavy cosmic-ray nuclei has observed one possible actinide nucleus and some ...
We report here an analysis that, for the first time, systematically normalizes the data from the HEA...
The HEAO-3 Heavy Nuclei Experiment has measured elemental abundances of ultraheavy cosmic rays near...
Data extraction and analysis of the LDEF Ultra Heavy Cosmic Ray Experiment is continuing. Almost twi...
Abundances relative to _(96)Fe have been derived for elements with charge, 2, in the range 32≤z≤40. ...
A passive, large‐area experiment for the detection of cosmic ray actinides on the lunar surface is d...
The relative abundances of elements in the charge ranges of 75 ≤ Z ≤ 79 (platinum) and 80 ≤ Z ≤ 83 (...
The suggestions that the source abundances of cosmic ray nuclei heavier then Fe differ significantly...