Techniques for suppressing anomalous response to vacuum ultraviolet radiation in the charged- particle lunar environment experiment.
Procedures to suppress anomalous response to vacuum UV radiation in lunar environment experiment
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Procedures to suppress anomalous response to vacuum UV radiation in lunar environment experiment
Design and performance of curved photomultiplier tube - effects of structural configuration on dead time and gain stability
Lithium doped silicon solar cells under electron irradiation and determination of semiconductor parameters
Equation describing statistically trapped particle motion under influence of fields varying in time and space
High temperature ion source developed for implantation and surface reactions of Ar, Pb, and Ga ions
Hall coefficient measurements of irradiated lithium doped solar cells
Determining solar absorptance stability of metallized Teflon second surface mirror thermal control coatings as function of electron, proton, and UV radiation dosage
Estimates of atomic concentration ionosphere from radar backscatter and rocket probe measurements of electron and ion temperatures and electron concentration
Electron and proton precipitation observations in auroral, polar cap and outer radiation zones by electrostatic analyzers on earth satellite Injun 5
Primary cosmic ray nucleonic component observation by scintillator-Cerenkov telescope on OGO 3 satellite
Glauber scattering amplitudes for atomic hydrogen excitation by electrons or protons, presenting closed form expressions requiring no numerical integration
Apollo 11 and 12 fines analysis, observing no quarks
The use of X-ray transition radiation to distinguish between protons and positrons of equal rigidity was investigated. A formula for the transition radiation spectrum from a medium-to-medium boundary was derived. The formation zone effect was found to limit the detection of transition radiation from ultrarelativistic particles. Curves showing the results of the spectrum calculations are presented.
An array of sensitive electrostatic analyzers was launched on the satellite INJUN 5 into a nearly polar, low altitude orbit. A series of three traversals of the northern auroral zone in the local evening sector on 3 December 1968 has provided high energy- and time-resolution observations of low-energy proton and electron intensities within the energy range 50 smaller than E smaller than 15,000 eV before, during and after a polar magnetic substorm. The region of high intensities of plasma-sheet electrons expanded dramatically during the substorm, extending 3.5 deg farther poleward and approximately 4.5 deg farther equatorward relative to that of the preceding pass.
The experiment package, consisting of seven Geiger-Mueller tubes as basic sensors, is described, including the instrumental characteristics and tube arrangements. The capabilities of surveying the absolute intensities, energy spectra, angular distributions of energetic electrons and protons in the Jupiter magnetosphere are discussed.
Demonstration that meaningful galactic and solar cosmic radiation measurements can be carried out on deep space missions. The radioisotopic thermoelectric generators (RTGs) which must be used as a source of power and perhaps of heat are a problem, but with proper separation from the experiments, with orientation, and with some shielding the damage effects can be reduced to an acceptable level. The Pioneer spacecraft are crucial in that they are targeted at the heart of Jupiter's radiation belts, and should supply the details of those belts. The subsequent Grand Tour opportunities can be selected for those periods which result in larger distances of closest approach to Jupiter if necessary.
Abstract missing.
The trajectory of the particle is made visible under a microscope by the accumulation of metallic silver at regions of the lattice damaged by the particle. This decoration of the particle track is accomplished by exposure of the crystal to light. The decoration of normally present lattice imperfections such as dislocations can be suppressed by the addition to the crystal of less than ten parts per million of a suitable polyvalent metal impurity. An account of some preliminary attempts to grow thin single crystals of AgCl is given also, and suggestions for a more refined technique are offered.