1961-1964 balloon observations of cosmic rays.
Low energy galactic cosmic radiation studies by high altitude balloon flights carrying nuclear emulsions, including solar activity, energy and intensity spectra, etc
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Low energy galactic cosmic radiation studies by high altitude balloon flights carrying nuclear emulsions, including solar activity, energy and intensity spectra, etc
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
Balloon-borne Cerenkov scintillation counter measurements of energy spectra of primary cosmic radiation heavy nuclei at various geomagnetic latitudes
Skyhook balloon flight Geiger counter cosmic ray monitor measurements of energy and charge spectra of galactic rays at solar minimum
Balloon flight experiment to search for celestial sources of X-rays in energy range 20 to 58 kev
Possible enhancement to low-energy atmospheric proton flux induced by passage of Ikeya-Seki comet examined, using balloon-borne scintillation counter and pulse height analysis techniques
Cosmic X-ray source near direction of north galactic pole, noting empirical results from balloon observations
Balloon-borne spark chamber observations of cosmic gamma rays from 30 to 500 mev
High altitude balloon-top measurements of cosmic dust
Proton and electron balloon measurements of splash and re-entrant cosmic ray albedo
Spurious balloon behavior and measurement of wind profiles
Eole experiment - weather satellite used to follow ceiling balloons with radioelectric responder
Extraterrestrial dust in stratospheric sampling collected by balloon-borne probe
Balloon observation of thermal radio emission of molecular oxygen in terrestrial atmosphere
Fast neutron latitude variations in atmosphere during solar minimum measured by high-altitude balloons, noting neutron leakage into space
Instrumental and observational aspects of balloon X-ray astronomy involving position, angular size, intensity and spectral measurements of X-ray sources
Energy spectrum of cosmic ray heavy nuclei, using stack of nuclear emulsions exposed during Quiet Sun on balloon flight