Two OSO's scheduled in series
Orbiting Solar Observatories OSO-E and OSO-D for studying Sun influence on Earth atmosphere
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Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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Orbiting Solar Observatories OSO-E and OSO-D for studying Sun influence on Earth atmosphere
Solar neutron transport in Earth atmosphere from neutron spectral measurements
History and stability of earth atmosphere
Two documents describe a proposed Earth-atmosphere observatory to orbit the Sun at the Sun-Earth L2 Lagrange point -- a point of unstable equilibrium in the shadow of the Earth, about 1.5 million km from the Earth along an outward projection of the Earth-Sun axis. The observatory would comprise two spacecraft flying in precision formation: (1) a primary-aperture spacecraft, from which would be deployed a 25-m diameter membrane primary mirror aimed at the Earth, and (2) a secondary-telescope spacecraft at the focal plane of the primary mirror, 125-m distant along the axis towards the Earth. The secondary telescope would be aimed at the primary mirror and slowly rotated to scan the focused annular image of the visible illuminated portion of the Earth's atmosphere during continuous occultation of the Sun.
Radiative heating of vehicles entering the earths atmosphere
Fast neutrons in earth atmosphere - balloon flights
What is Earth-GRAM? Provide monthly mean and standard deviation for any point in atmosphere; Monthly, Geographic, and Altitude Variation. Earth-GRAM is a C++ software package; Currently distributed as Earth-GRAM 2016. Atmospheric variables included: pressure, density, temperature, horizontal and vertical winds, speed of sound, and atmospheric constituents. Used by engineering community because of ability to create dispersions inatmosphere at a rapid runtime; Often embedded in trajectory simulation software. Not a forecast model. Does not readily capture localized atmospheric effects.
Electromagnetic wave transmission in earth atmosphere from 3 kHz to 3000 THz with emphasis on earth to space paths up to Jan. 1970
Efficiency of solar cell power systems outside the earths atmosphere
Geometric attenuation of hydromagnetic waves in the earths atmosphere
Spacecraft piloted entry into earth atmosphere at parabolic velocity investigated on fixed base analog simulator
Free oscillation frequencies of earth atmosphere
Solar and stellar radiations above earth atmosphere
Strongly damped gravity waves in earth atmosphere evidenced by rocket sounding
Ambient pressure, temperature, and density measurements for earth atmosphere by rocket probe instrumentation
Solar radiation transmitted and reflected by earth atmosphere, solving absorption and scattering by computer programs
Monte Carlo method used for calculating reflected and transmitted radiance of earth atmosphere
Electronic digital computers for calculation of acoustic-gravity wave propagation in earth atmosphere