Proton, helium, and medium nuclei energy spectra have been measured from the Explorer 35 satellite for a recent solar flare. Above 2 MeV/nucleon these spectra are based upon single and dual parameter pulse height analysis in addition to threshold rate counting. Pulse height analysis of medium nuclei is assigned a high priority for telemetry readout so that telemetry does not become saturated by the high proton intensity. In this manner the number of pulse height analyzed medium nuclei has been increased by a factor of approximately 200. Individual medium nuclei have been resolved in the energy interval 8 - 23 MeV/nucleon
A study of the composition and energy spectra of solar cosmic rays from the Nov. 12, 1960 solar flar...
The cosmic-ray proton and helium spectra from 0.2 GeV nucleon^(-1) to about 200 GeV nucleon^(-1) hav...
Aims. Several experiments have reported observations on possible correlations between the flux of hi...
An approach to measuring charged spectra of solar cosmic rays is considered. These observations were...
The composition of energetic solar particles is reviewed for all solar events in which measurements ...
Using data from the Cosmic Ray Subsystem aboard the Voyager 1 and 2 spacecraft (Stone et al., 1977),...
The PHEBUS experiment aboard GRANAT observed γ-ray line emission and γ-ray continuum abo...
Relative abundances of energetic nuclei in the 4 July 1974 solar event are presented. The results sh...
The PHEBUS experiment aboard GRANAT observed γ-ray line emission and γ-ray continuum above...
Recordings on relativistic solar flare protons observed at Sanae, Antarctic, show that the percentag...
Solar flares are among the most energetic and interesting phenomena in the Solar system, releasing u...
We have studied a subset of the 11 June 1991 solar flare γ-ray data that we believe arise from soft ...
Energetic helium and heavy nuclei (Z ≥ 3) were detected in the July 18, 1961, solar particle e...
Observations of helium and heavier particles with energies below about 10 to 20 MeV/nucleon are disc...
An unusual spectral feature and anomalously large abundance of helium between 0.6 and approximately ...
A study of the composition and energy spectra of solar cosmic rays from the Nov. 12, 1960 solar flar...
The cosmic-ray proton and helium spectra from 0.2 GeV nucleon^(-1) to about 200 GeV nucleon^(-1) hav...
Aims. Several experiments have reported observations on possible correlations between the flux of hi...
An approach to measuring charged spectra of solar cosmic rays is considered. These observations were...
The composition of energetic solar particles is reviewed for all solar events in which measurements ...
Using data from the Cosmic Ray Subsystem aboard the Voyager 1 and 2 spacecraft (Stone et al., 1977),...
The PHEBUS experiment aboard GRANAT observed γ-ray line emission and γ-ray continuum abo...
Relative abundances of energetic nuclei in the 4 July 1974 solar event are presented. The results sh...
The PHEBUS experiment aboard GRANAT observed γ-ray line emission and γ-ray continuum above...
Recordings on relativistic solar flare protons observed at Sanae, Antarctic, show that the percentag...
Solar flares are among the most energetic and interesting phenomena in the Solar system, releasing u...
We have studied a subset of the 11 June 1991 solar flare γ-ray data that we believe arise from soft ...
Energetic helium and heavy nuclei (Z ≥ 3) were detected in the July 18, 1961, solar particle e...
Observations of helium and heavier particles with energies below about 10 to 20 MeV/nucleon are disc...
An unusual spectral feature and anomalously large abundance of helium between 0.6 and approximately ...
A study of the composition and energy spectra of solar cosmic rays from the Nov. 12, 1960 solar flar...
The cosmic-ray proton and helium spectra from 0.2 GeV nucleon^(-1) to about 200 GeV nucleon^(-1) hav...
Aims. Several experiments have reported observations on possible correlations between the flux of hi...