Limits to the distances of the quasi-stellar objects deduced from their absorption line spectra.
Red shifts from absorption line spectra of quasi- stellar objects, discussing energy generation mechanism
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Red shifts from absorption line spectra of quasi- stellar objects, discussing energy generation mechanism
Engineering design of transponder system for phase measurement of very low frequency signals
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Geomagnetic micropulsation measurements for magnetosphere and solar wind diagnostics
Solar wind and current sheet considered in determining shape of magnetosphere boundary and calculation of magnetic field lines
Computer approach to first order planetary theory using perturbation calculation in rectangular coordinates
Lunar magnetic field measurements by Mariner 4 near sun-moon line extension, discussing search for lunar wake
Magnetopause boundary between shocked streaming solar plasma and geomagnetic tail observed at lunar orbit by magnetometer on Explorer 35
Nucleated organisms divergence from bacteria compared to nucleated organisms divergence into separate kingdoms by analysis of genetic changes in cytochrome c and transfer RNA
Observational errors effects on surface waves resolution, describing shear velocity determination in crust and mantle from observed waves
Comparing results of reentry plasma diagnostic experiment at 25,000 ft/sec with flow-field values at four locations on spacecraft
Solving exact gas dynamic equations for supersonic flows far from axis of slender lifting bodies
Design and construction of cryopump is reported that feeds from primary source to cool component up to 30 ft from source. Liquid oxygen or nitrogen is gravity fed through loop system to copper fibers enclosing component at room temperature where fluid boils, cools object, vaporizes and recycles through tubing loop.
During the partial lunar eclipse of August 17, 1970, four intense, transient bursts of kV-energy positive ions were detected at the lunar surface by the Rice University ALSEP Suprathermal Ion Detector Experiment. The eclipse happened to occur during a main-phase geomagnetic storm while the moon was within a few earth radii of the calculated position of the neutral sheet. The two most intense ion bursts were each followed roughly one-half hour later by the sudden onset of a several thousand gamma polar magnetic substorm at the earth's surface. Two smaller ion enhancements were also followed by smaller magnetic disturbances. This observation is interpreted in terms of a downstream escape of plasma-sheet particles associated with the substorm growth phase.
During the last five years, much progress has been made in the understanding of sky-wave backscatter. An explanation of the various interacting phenomena is presented, as is a review of the current state of knowledge reflecting recent advances in observational methods and analytic techniques. New narrow-beam antennas, coupled with signal modulations that permit fine resolution in time delay, are beginning to yield information concerning the character of the scatterers, which now can be separately discerned. These narrow beams also permit study of polarization fading from small regions, and this shows promise as a means for learning the distant sea state. Doppler shifts of a fraction of a hertz on signals of tens of megahertz are separable, permitting isolation of sea returns from ground returns by virtue of the Doppler effect resulting from sea-wave speed; this also suggests a potential sea-monitoring principle. Despite these advances, there is little practical application of sky-wave backscatter as a means of environmental monitoring. This lack is attributed to the large remaining gaps in our understanding of the echoes and our inability to interpret the forms of data that can be acquired with equipment of reasonable cost.
Evaluation of plasma data from the Apollo 14 charge particle lunar environment experiment showing that, contrary to previously published analyses, the plasma sheet does not extend to the lunar orbit with a thickness of 8 earth radii. Two electron spectral types are observed: (1) low-energy photoelectrons with no statistically significant medium and high energy fluxes, and (2) double-peaked medium- and high-energy electrons. The second type is observed either coincident with auroral substorms or at the center of the tail during quiet times. These spectra are one to several orders of magnitude less intense than plasma sheet spectra measured near 20 earth radii.
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