Gamma-ray astronomy results at balloon altitudes
Astronomical gamma ray emission measurement by balloon-borne spark chamber, presenting results for discrete and diffuse sources and albedo intensities
Engineering topics
Publications and source records attributed to Fichtel, C. E..
Astronomical gamma ray emission measurement by balloon-borne spark chamber, presenting results for discrete and diffuse sources and albedo intensities
Cosmic ray positrons and negatrons differential intensities near north geomagnetic pole from balloon flight measurements, noting solar modulation effects
Relativistic cosmic rays nuclei abundances from Gemini 11 flight
Gamma ray astronomical point sources by balloon flight and satellite observation, discussing detector system and telescope for flux and energy spectrum
Gamma ray astronomy using balloon-borne telescope with digitized spark chamber
Chemical composition of relativistic cosmic rays detected above atmosphere
Balloon flight detection of gamma ray point sources
Balloon measurements of cosmic ray positron and negatron intensities near North Pole
Abundances and composition of relativistic cosmic rays observed on Gemini 11 flight
Iron group nuclei abundance relative to oxygen determined for solar cosmic ray event of 2 September 1966
High altitude balloon flight results of gamma rays digitized spark chamber telescope
Gamma ray telescope development for balloon-borne astronomy in search for discrete gamma sources and supernova explosions
Source, composition, and propagation of nuclear components of cosmic rays
Detector and spark chamber systems for gamma ray astronomy in first-generation experiments
Primary cosmic ray nuclei studies during Gemini 2 flight by nuclear emulsion detector with time resolution capability, describing experiment design and equipment operation
Cosmic ray propagation, discussing interstellar matter effect on composition and diffusion effect necessary to study radiation models
Gamma ray telescope utilizing wire spark chamber for balloon borne astronomy
Heavy nuclei detected in September 2, 1966 solar particle event, measuring proton, helium and heavy nuclei energy spectra