Trapped electron time histories for L equals 1.18 to L equals 1.30
Numerical integration of Fokker-Planck equation used to predict decay time of electrons injected into geomagnetic field by nuclear explosion
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Numerical integration of Fokker-Planck equation used to predict decay time of electrons injected into geomagnetic field by nuclear explosion
Soviet scientists contributions to jet engineering development in 1930s
Pressure - time computations of sonic boom shock wave acting on window glass and walls of building
Cyclotron radius, magnetospheric boundary and Debye length scaling parameters for magnetospheric cavity arising from solar wind- induced geomagnetic storm and visibility of quasi- Van Allen belts
Microwave reflectometer instrumentation for Ames light-gas guns, measuring time-distance values of projectiles during acceleration
Program computes the thermal environment of a spacecraft in a lunar orbit. The quantities determined include the incident flux /solar and lunar emitted radiation/, total radiation absorbed by a surface, and the resulting surface temperature as a function of time and orbital position.
OSO-II data on solar activity and electromagnetic radiation
Influence of shock or stress events induced by underground nuclear explosions on low temperature thermoluminescence of halite
Thermal evolution of Earth, Mars, and Moon
Calculating past states of earth-moon system based on three time scales for dynamical change
X-ray diffraction and metallographic investigation show iron meteorites shock at pressures of at least 130 kbar
Ti stress corrosion in nitrogen tetroxide, detailing investigative techniques
Cooling rates for Widmanstatten pattern formation in iron meteorites used to obtain data on parent meteorite bodies
Temperature profiles of primitive terrestrial planets, discussing gravitational energy, radioactive isotope, internal heat redistribution and radiative transfer effects
Diurnal variation of radar angel activity from cirrus clouds and clear atmosphere region at three wavelengths
Solar activity model provides information on plages, sunspots, filaments, and flares. The model enables scheduling, which will indicate the time periods when solar experiments can be conducted. Data were collected at various locations throughout the world and recorded on tape for the computer.
Review of highway and runway traction studies
Simulation of service load distributions using digital computers with FORTRAN 4 program