OGO program - Bibliography
Abstracts and experiment descriptions of OGO I, II, III, E, and F - Bibliography
BIBLIOGRAPHY↗
Engineering topics
Ludwig, G. H.
Publications and source records attributed to Ludwig, G. H..
Relative advantages of small and observatory type satellites
Weight and volume capability, celestial orientation, data handling and storage, telemetry, and reliability of Explorer type satellites and orbiting type observatories
COMPONENT RELIABILITY↗
Instrumentation for space physics.
Satellite instrumentation, discussing data handling systems, cosmic ray detection, signal and information processing, etc
DATA HANDLING SYSTEM↗
The multiply charged primary cosmic radiation at solar minimum, 1965.
Primary cosmic ray charge and energy spectra for helium through oxygen during 1965 minimum solar modulation effect
SOLAR ACTIVITY EFFECT↗
Satellite observations of MeV phenomena related to the solar wind. Explorer-12 observations. IMP observations of primary 3-MeV electrons
Explorer XII and IMP satellite observations of MeV phenomena related to solar wind
EXPLORER XII SATELLITE↗
Satellite observations of Mev phenomena related to the solar wind - Explorer-12 observations. IMP observations of primary 3-mev electrons.
Solar wind observations with Explorer XII and IMP, noting periodic fluctuations in solar proton flux and detection of 3 mev electrons of interplanetary origin
INTERPLANETARY SPACE↗
Galactic cosmic rays at solar minimum, 1965.
Skyhook balloon flight Geiger counter cosmic ray monitor measurements of energy and charge spectra of galactic rays at solar minimum
SOLAR COSMIC RAY↗
Relative advantages of small and observatory type satellites.
Explorer type compared to Orbiting Observatory type satellites regarding weight, volume, reliability, data transmission, power, etc
OAO↗
The multiply-charged primary cosmic radiation at solar minimum, 1965
Primary cosmic ray charge and energy spectra determination for helium through neon during solar minimum
ENERGY SPECTRUM↗
Detection of interplanetary 3- to 12-mev electrons
Observations of interplanetary 3- to 12-MeV electrons with IMP-I - Explorer XVII SATELLITE - galactic versus solar evolution
EXPLORER XVII SATELLITE↗
Measurement of low energy primary cosmic ray protons on imp 1 satellite
IMP-I satellite telescopic measurements of low energy primary cosmic ray protons
COSMIC RAY↗
Relative advantages of small and observatory type satellites
Small Explorer and large orbiting observatory classes of scientific satellites
EXPLORER SATELLITE↗
Results from the imp 1 gm counter telescope experiment.
Cosmic ray intensity variations measured by GM COUNTER telescope onboard Imp I satellite for study of interplanetary medium
COSMIC RADIATION↗
Relative advantages of small and observatory type satellites.
Explorer type compared to Orbiting Observatory type satellites regarding weight, volume, reliability, data transmission, power, etc
SATELLITE CONFIGURATION↗
Some results from the IMP-1 GM cosmic ray detector
IMP-1 cosmic ray detector design and intensity measurements
RADIATION DETECTOR↗
Some results from the imp-1 gm cosmic ray detector
Explore the source record for details and available documents.
Balasubrahmanyan, V. K.↗
Measurement of low energy primary cosmic ray protons on imp-1 satellite
Intensity and energy spectra determination of primary cosmic ray protons by telescope aboard Explorer XVIII satellite
INTENSITY↗
Detection of interplanetary 3- to 12-mev electrons
Detection and observations of interplanetary electrons with scintillator telescope aboard Explorer XVIII satellite
EXPLORER XVIII SATELLITE↗