Ionization equilibrium and radiative cooling of a low-density plasma.
Ionization equilibrium and radiative cooling of high temperature low density plasma, noting cosmic gas cooling curve of line emission from oxygen ion transitions
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Ionization equilibrium and radiative cooling of high temperature low density plasma, noting cosmic gas cooling curve of line emission from oxygen ion transitions
Rotating neutron stars, pulsars and cosmic X ray sources, accounting for large and small diameter sources by rotating neutron star losing mass in magnetic field
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Lateralization and detection of signals under antiphasic noise masking measured at various SNR levels
Formaldehyde rotational transition hyperfine components measured by molecular beam maser
Crab Nebula filametary system, examining excitation conditions in terms of ionization and heating by HF radiation
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Tool cuts multiple slits up to 3 in. long between conductors of flat conductor cables up to 3 in. wide to prepare them for termination on terminal boards or in multipin connectors.
Space suit body heat exchanger design composed of thermal conductance yarn and liquid coolant loops
Design and development of flexible tunnel for use by spacecrews in performing extravehicular activities
Final data analysis of grazing incidence of solar X ray telescope experiment of OSO- 4 satellite
Computer controlled mass spectrometer system, processing spectral information data for on-line graphic system output
Supernova explosion or solar outburst theory of climatic effects on mass extinction of organisms at Cretaceous-Tertiary boundary
Extragalactic cosmic X ray sources at high galactic latitude from sounding rocket experiments, correlating with galactic clusters
Vela X supernova remnant blast wave model and Gum Nebula formation, discussing kinetic and rotational energy transformation into radiation
Solar coronal X ray spectrum calculation of high- temperature low-density plasma, considering line emission from electron collisional excitation and radiation
Formaldehyde transitions in ground and excited states at 6 cm, attaining line widths and hyperfine structure at 1-3 kHz
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