The OGO-V plasma wave detector - Instrumentation and in-flight operation.
OGO 5 spacecraft detector instrumentation for measuring electrostatic and electromagnetic waves electric fields with coupled antennas, describing in-flight operation
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OGO 5 spacecraft detector instrumentation for measuring electrostatic and electromagnetic waves electric fields with coupled antennas, describing in-flight operation
Low energy proton detector instrumentation as plasma probe on explorer x
Engineering analyses on Surveyor lunar dust particle detector instrumentation, and ground support equipment
Portable instrument passes light from helium-neon laser at a wavelength of 3.39 microns through the atmosphere being monitored and measures attenuation of the laser beam. Since beam attenuation is due almost exclusively to absorption of radiation by hydrocarbons, a quantitative measure of their concentration is available.
Design, fabrication, and testing of breadboard model of instrument for detection of extraterrestrial life by means of optical rotatory dispersion
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Charge-sensitive amplifier for use with solid state radiation detectors in spacecraft instrumentation system
Element abundances in igneous rocks measured by instrumental neutron activation using high resolution lithium drifted germanium detectors
Nimbus High Resolution Infrared Radiometer /HRIR/, subsystem, calibration, and flight performance
Cadmium sulfide radiation detector for satellites
The StarBurst Multimessenger Pioneer is a small satellite mission serving as a wide-field gamma-ray observatory designed to capture the initial emissions of short gamma-ray bursts, electromagnetic signatures of neutron star mergers. This paper presents the final thermal design and analysis of the StarBurst Instrument, comprising the bus-to-instrument interface plate, control electronics, and twelve crystal detector units, which form the core of the mission’s science capability. The passive thermal control system design requires consideration of restrictive keep-out zones, unknown orbital parameters, and narrow temperature limits of the detectors. Also summarized is the instrument level thermal vacuum cycle test, correlated model refinements, and updated model results. Following successful completion of the instrument test campaign, the hardware was integrated with the spacecraft bus for spacecraft level testing, including additional thermal vacuum testing. The results from the spacecraft level thermal vacuum test will further inform the instrument thermal model, ensuring accurate flight temperature predictions. StarBurst launches as a secondary payload in 2027 and has a mission duration of at least one year.
The StarBurst Multimessenger Pioneer is a small satellite mission serving as a wide-field gamma-ray observatory designed to capture the initial emissions of short gamma-ray bursts, electromagnetic signatures of neutron star mergers. This paper presents the final thermal design and analysis of the StarBurst Instrument, comprising the bus-to-instrument interface plate, control electronics, and twelve crystal detector units, which form the core of the mission’s science capability. The passive thermal control system design requires consideration of restrictive keep-out zones, unknown orbital parameters, and narrow temperature limits of the detectors. Also summarized is the instrument level thermal vacuum cycle test, correlated model refinements, and updated model results. Following successful completion of the instrument test campaign, the hardware was integrated with the spacecraft bus for spacecraft level testing, including additional thermal vacuum testing. The results from the spacecraft level thermal vacuum test will further inform the instrument thermal model, ensuring accurate flight temperature predictions. StarBurst launches as a secondary payload in 2027 and has a mission duration of at least one year.
Trapped radiation detector for Mariner C program
Many of the spacecraft launched thus far have carried detectors for investigating cosmic rays, solar protons, solar plasmas, and the geomagnetically trapped radiation. These detectors, which will find continued application in the future, include ion chambers; proportional, Geiger-Muller, scintillation, Cerenkov, and solid state detectors; ion collectors; and nuclear emulsions. The instrumentation required to condition the signals from these detectors prior to telemetering is steadily growing more complex in order to permit more meaningful measurements. This report describes a number of instrumentation elements typical of the present state of the art, and a present-generation three-detector system which illustrates the integration of such basic elements into a complex system.
Directional neutron detector using liquid scintillator for low mev energy range for rocket and satellite experiments
Pioneer VI detector to measure degree of anisotropy of cosmic radiation at various energy ranges
Design of a double-focusing mass spectrometer for quantitative measurement of atmospheric elements for use in earth satellites
Furnace system operating at 2000 degrees K for determination of IR absorption of high temperature gases