An approach to measuring charged spectra of solar cosmic rays is considered. These observations were made by a telescope on the IMP 6 satellite. The charge range was extended beyond charge 2 up to charge 26, and the energy range was extended to lower energies. The experiment preferentially selects rare events above charge 2 and gives them top priority for telemetry readout, thus breaking the monopoly that protons and helium nuclei otherwise would have on the telemetry. This effectively increases the number of nuclei observed above charge 2 by a factor of several hundred
Measurements from the Heavy Nuclei Experiment (Binns et al. 1981a) aboard the HEAO-3 satellite have...
In 1976, 1977 and 1978, three balloon flights were conducted to measure the energy spectra of cosmic...
A study of the composition and energy spectra of solar cosmic rays from the Nov. 12, 1960 solar flar...
The composition and energy spectra of cosmic rays above 1.6 nJ (10 GeV) on balloons and ultimately o...
The composition of energetic solar particles is reviewed for all solar events in which measurements ...
Experimental results from the balloon borne ionization spectrometer have enabled the extension of th...
Proton, helium, and medium nuclei energy spectra have been measured from the Explorer 35 satellite f...
The Cosmic Ray System (CRS) experiment on board each of the Voyager 1 and 2 spacecraft consists of f...
A group collaboration was made in the development of the Bristol University Gas Spectrometer number ...
A definitive study of the elemental abundances of nuclei over the charge range of 20 ≤ Z ≤ 100 requi...
Using data from the Cosmic Ray Subsystem aboard the Voyager 1 and 2 spacecraft (Stone et al., 1977),...
The composition of the nuclear component of the cosmic radiation was studied to yield information co...
A detailed study of the charge composition of heavy solar cosmic rays measured in the January 25, 19...
The general features of the solar particle composition now seem to be clear. The two most abundant c...
Composition and energy spectra of solar cosmic rays - november 12, 1960 - solar flare, hydrogen, hel...
Measurements from the Heavy Nuclei Experiment (Binns et al. 1981a) aboard the HEAO-3 satellite have...
In 1976, 1977 and 1978, three balloon flights were conducted to measure the energy spectra of cosmic...
A study of the composition and energy spectra of solar cosmic rays from the Nov. 12, 1960 solar flar...
The composition and energy spectra of cosmic rays above 1.6 nJ (10 GeV) on balloons and ultimately o...
The composition of energetic solar particles is reviewed for all solar events in which measurements ...
Experimental results from the balloon borne ionization spectrometer have enabled the extension of th...
Proton, helium, and medium nuclei energy spectra have been measured from the Explorer 35 satellite f...
The Cosmic Ray System (CRS) experiment on board each of the Voyager 1 and 2 spacecraft consists of f...
A group collaboration was made in the development of the Bristol University Gas Spectrometer number ...
A definitive study of the elemental abundances of nuclei over the charge range of 20 ≤ Z ≤ 100 requi...
Using data from the Cosmic Ray Subsystem aboard the Voyager 1 and 2 spacecraft (Stone et al., 1977),...
The composition of the nuclear component of the cosmic radiation was studied to yield information co...
A detailed study of the charge composition of heavy solar cosmic rays measured in the January 25, 19...
The general features of the solar particle composition now seem to be clear. The two most abundant c...
Composition and energy spectra of solar cosmic rays - november 12, 1960 - solar flare, hydrogen, hel...
Measurements from the Heavy Nuclei Experiment (Binns et al. 1981a) aboard the HEAO-3 satellite have...
In 1976, 1977 and 1978, three balloon flights were conducted to measure the energy spectra of cosmic...
A study of the composition and energy spectra of solar cosmic rays from the Nov. 12, 1960 solar flar...