Add to ORKGAbundances relative to _(96)Fe have been derived for elements with charge, 2, in the range 32≤z≤40. With a resolution better than 0.5 charge unit at Z=38, we resolve _(37)Rb from _(38)Sr and use the Rb/Sr ratio to place a limit on the r-proccss enhancement of the cosmic ray source material in this charge range
The HEAO 3 detector of heavy cosmic-ray nuclei has observed one possible actinide nucleus and some ...
We review current work on the abundances of the ultraheavy elements in the cosmic radiation, those w...
The Heavy Nuclei Experiment on (HEAO-3) high energy astronomy observatory 3 uses a combination of io...
Abundances relative to _(96)Fe have been derived for elements with charge, 2, in the range 32≤z≤40. ...
Measurements from the Heavy Nuclei Experiment (Binns et al. 1981a) aboard the HEAO-3 satellite have...
We report here an analysis that, for the first time, systematically normalizes the data from the HEA...
Analysis of a new, higher resolution data set from the Heavy Nuclei Experiment on the HEA0-3 spacec...
Individual elements in the cosmic radiation of even atomic number (Z) in the interval 26 ≤ Z ≤ 40 ha...
The HEAO-3 Heavy Nuclei Experiment has measured elemental abundances of ultraheavy cosmic rays near...
Individual elements in the cosmic radiation of even atomic number (Z) in the interval 26 ≤ Z ≤ 40 ha...
Observations of the abundances of elements of charge 62 or Z or = 73 in the cosmic radiation from th...
The Heavy Nuclei Experiment on HEAO 3 included ionization chambers and a Cherenkov detector. For nu...
Using the relativistic rise of energy loss as a measure of energy, we have determined the energy de...
Isotope measurements of cosmic ray nuclei beyond the Fe peak are considered, using the charge region...
A definitive study of the elemental abundances of nuclei over the charge range of 20 ≤ Z ≤ 100 requi...
The HEAO 3 detector of heavy cosmic-ray nuclei has observed one possible actinide nucleus and some ...
We review current work on the abundances of the ultraheavy elements in the cosmic radiation, those w...
The Heavy Nuclei Experiment on (HEAO-3) high energy astronomy observatory 3 uses a combination of io...
Abundances relative to _(96)Fe have been derived for elements with charge, 2, in the range 32≤z≤40. ...
Measurements from the Heavy Nuclei Experiment (Binns et al. 1981a) aboard the HEAO-3 satellite have...
We report here an analysis that, for the first time, systematically normalizes the data from the HEA...
Analysis of a new, higher resolution data set from the Heavy Nuclei Experiment on the HEA0-3 spacec...
Individual elements in the cosmic radiation of even atomic number (Z) in the interval 26 ≤ Z ≤ 40 ha...
The HEAO-3 Heavy Nuclei Experiment has measured elemental abundances of ultraheavy cosmic rays near...
Individual elements in the cosmic radiation of even atomic number (Z) in the interval 26 ≤ Z ≤ 40 ha...
Observations of the abundances of elements of charge 62 or Z or = 73 in the cosmic radiation from th...
The Heavy Nuclei Experiment on HEAO 3 included ionization chambers and a Cherenkov detector. For nu...
Using the relativistic rise of energy loss as a measure of energy, we have determined the energy de...
Isotope measurements of cosmic ray nuclei beyond the Fe peak are considered, using the charge region...
A definitive study of the elemental abundances of nuclei over the charge range of 20 ≤ Z ≤ 100 requi...
The HEAO 3 detector of heavy cosmic-ray nuclei has observed one possible actinide nucleus and some ...
We review current work on the abundances of the ultraheavy elements in the cosmic radiation, those w...
The Heavy Nuclei Experiment on (HEAO-3) high energy astronomy observatory 3 uses a combination of io...