Solar cosmic ray heavy nuclei and the 18th July 1961 event.
Balloon-borne nuclear emulsion detection of solar cosmic ray heavy nuclei during solar burst
Engineering topics
Publications and source records attributed to Guss, D. E..
Balloon-borne nuclear emulsion detection of solar cosmic ray heavy nuclei during solar burst
Balloon-borne nuclear emulsion detection of finite fluxes of low energy cosmic ray heavy nuclei and interstellar cosmic radiation propagation
Cosmic ray nuclei flux with charges greater than that of helium at energies below balloon-borne experiments cutoff value
Nuclear emulsion measurements on particle populations in space using sounding rockets and Gemini spacecraft
Low energy cosmic ray heavy nuclei examination by sounding rocket
Heliographic longitude of solar flares producing energetic particles
Low energy galactic cosmic ray modulation
Spectral variation of low energy galactic cosmic ray protons and helium nuclei measured by balloon flights
Intensities and energies of solar cosmic ray particles detected near earth
Flux and energy spectrum of solar hydrogen, helium and heavy nuclei is measured during three rocket firings, using nuclear emulsions techniques
Composition and energy spectra of solar cosmic rays - november 12, 1960 - solar flare, hydrogen, helium, and nuclei
Data on solar proton intensities and spectra, obtained by means of nuclear emulsions carried by high-altitude balloons
Energy spectra of cosmic ray hydrogen and helium nuclei determined from nuclear emulsions flown in high altitude balloon
Study of cosmic-ray emission from a solar flare based on nuclear-emulsion data recovered from rocket probes
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A study of hydrogen, helium and heavy nuclei in the nov. 1960 solar cosmic ray event
Energy spectra, intensity and radiation of cosmic rays from solar proton events