Apollo helmet dosimetry experiments Final report
Procedure for measuring heavy cosmic ray particles directly incident on spacecrews
Engineering topics
Publications and source records attributed to Comstock, G. M..
Procedure for measuring heavy cosmic ray particles directly incident on spacecrews
Rock particle tracks of primary cosmic rays, spallation recoil nuclei, nuclear fission and solar wind ions, observing time scale multiple soil orientation
Cosmic ray nuclei energy spectra and abundances above 20 Mev/nucleon determined by OGO-1 satellite experiment, considering He, B, C, N, O, Ne, Mg, Si, Mn, Fe, Co and Ni
Low energy multiply charged cosmic ray nuclei propagation and source characteristics, considering two component model based on OGO satellite measurements
Low energy cosmic ray nuclei propagating in interstellar space analyzed by telescope onboard OGO 1
Energy spectra and abundances of elements He through Si of galactic cosmic ray above 20 mev per nucleon in nuclear charge range between 2 and 26
Chemical abundances and energy spectra of nuclei in galactic radiation measured in interplanetary space by OGO-I satellite