Study of a small solar probe /sunblazer/. part i- radio propagation experiment
Electron density of solar corona using radio propagation with coherent multifrequency transmissions from small heliocentric orbiting satellite
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Electron density of solar corona using radio propagation with coherent multifrequency transmissions from small heliocentric orbiting satellite
Branch-fed variable-phase 20 to 55 mc antenna array for radar studies of Moon, cislunar gas and solar corona
Collisional excitation of autoionizing levels in solar corona
Stability of dilute gas in mechanical and thermal equilibrium with application to nongravitational condensation phenomena in astronomy, particularly solar corona
Type III and IV bursts in solar corona - brightness distribution of source
Doppler characteristics of radar echoes reflected by solar corona
Nonlinear treatment of prominence condensation from solar corona by thermal instability
Collisional excitation of autoionizing levels in solar corona
Transient anisotropic cosmic ray increase during recovery phase of Forbush decrease due to reflection from receding blast wave and co-rotating shock wave formed during explosive heating of solar corona
Solar X rays and radio emission by free-free electron transitions in solar corona
Collisional ionization effects on fractional concentration of atoms of particular ionization in low density plasma, noting ionization equilibrium in solar corona
Thermal instability mechanism for quiescent solar prominence formation by condensation from solar corona, noting condensation inhibition by free electrons heat conduction
Oxygen VI emission from sun, calculating ionization equilibrium of O at various temperatures and contributions from solar corona and transition regions
Conceptual design of Sunblazer space probe for determining electron density of solar corona
Approximative line intensity ratios of iron 17 in solar corona