Resolving the High‐Latitude Ionospheric Irregularity Spectra Using Multi‐Point Incoherent Scatter Radar Measurements
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Explore the source record for details and available documents.
Explore the source record for details and available documents.
Explore the source record for details and available documents.
Explore the source record for details and available documents.
Explore the source record for details and available documents.
Dense high-temperature plasma produced by 30- kjoule theta pinch examined by IR maser-excited coupled resonator system
Computer program computes temperature distribution as a function of time in a given body which has been subdivided into a network of nodes. Thermal resistances and capacitances may be computed from nodal geometry.
Dense high temperature plasma produced by 30- kjoule theta pinch examined by IR maser-excited coupled resonator system
Waveforms analyzer for mixtures of exponentially damped sine waves, noting application to interferometer curves in plasma wave propagation
Development of method for synchronizing clocks at several ground stations based on signals received from spacecraft or satellites
Spectrographs for measuring hydrogen H beta line spectral shape and determining electron density of transient plasma
Magnetospheric VLF banded emissions spectral analysis, investigating OGO-5 data by high time resolution spectral techniques
Diurnal temperature variations in the upper atmosphere are caused by heating resulting from the absorption of solar energy by ozone near the stratopause and by water vapor in the troposphere. Theoretical temperature variations given as a function of time and height show a discrepancy for the maximum temperature variation. A comprehensive set of acoustic grande soundings establish phase changes with altitude in agreement with the theory although times of maximum and minimum are not aligned at all altitudes.
Some preliminary spectroscopic results of an investigation of the radiation from bulk specimens of burning titanium are presented. The use of larger stationary specimens is shown to have considerably eased some of the experimental difficulties associated with metal combustion research and to approximate more closely the conditions prevailing in large-scale accidental metal fires.
The Population 2 sub-dwarf star mu Cas was photographed, yielding elongated images from which the separation magnitude of the unseen component can be derived.
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