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  • 11
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    Cosmic radio noise intensity from 0.45 to 3.0 MHz observed by the ATS II satellite. (1969)
    In:  Other Sources
    Details
    Publication Date: 2011-08-12
    Description: Cosmic radio noise intensity measurements by ATS 2 satellite-borne radiometer
    Keywords: SPACE SCIENCES
    Type: ; UGREVUE(
    Format: text
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    NASA TECHNICAL REPORTS
  • 12
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    The spectrum of the cosmic radio background between 0.4 and 6.5 MHz. (1969)
    In:  Other Sources
    Details
    Publication Date: 2011-08-12
    Description: Cosmic radio background noise spectrum near north galactic pole based on Radio Astronomy Explorer satellite experiments
    Keywords: SPACE SCIENCES
    Type: ; YAL SOCIETY (
    Format: text
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    NASA TECHNICAL REPORTS
  • 13
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    Radioastronomy from space (1970)
    In:  Other Sources
    Details
    Publication Date: 2011-08-16
    Description: Spaceborne long wavelength radio astronomy, proposing lunar orbit and beyond Pluto observatories to reduce magnetospheric and interplanetary plasma effects
    Keywords: SPACE SCIENCES
    Type: ; 83 (
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  • 14
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    Radio physics of the outer solar system. (1973)
    In:  Other Sources
    Details
    Publication Date: 2011-08-16
    Description: The remote sensing of low frequency nonthermal radio emission is the astronomy of field and particle phenomena. Observations conducted from space lead to information about the composition and dynamic processes occurring in planetary magnetospheres as well as within the interplanetary and interstellar medium. The potential of this technique is demonstrated by considering observations obtained from earth orbit missions.
    Keywords: SPACE SCIENCES
    Type: Space Science Reviews; 14; Mar
    Format: text
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  • 15
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    Rocket measurements of cosmic-noise intensities below 5 Mc/s. (1965)
    In:  Other Sources
    Details
    Publication Date: 2011-08-11
    Description: Cosmic radio-noise intensities below 5 mc measured by rocket probe
    Keywords: SPACE SCIENCES
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    NASA TECHNICAL REPORTS
  • 16
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    The structure and circulation of the deep Venus atmosphere (1974)
    In:  Other Sources
    Details
    Publication Date: 2011-08-16
    Description: A simple model for the structure of a nonrotating Hadley regime in an atmosphere with large thermal inertia is developed. The radiative fluxes are estimated by using a linearization about the radiative equilibrium state, and the dynamical fluxes are estimated by using scaling analysis. The requirement that differential heating by these fluxes be in balance in both the meridional and vertical directions leads to two equations for the mean static stability and meridional temperature contrast. The solution depends on two parameters: the strength of the radiative heating, as measured by the static stability of the radiative equilibrium state; and the ratio of the time it takes an external gravity wave to traverse the atmosphere to the time it would take the atmosphere to cool off radiatively. It is shown that it is not necessary to invoke convection to explain the approximate adiabatic lapse rate in the Venus atmosphere, but a greenhouse effect is necessary to explain the high surface temperatures.
    Keywords: SPACE SCIENCES
    Type: Journal of the Atmospheric Sciences; 31; Sept
    Format: text
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  • 17
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    The sun. (1965)
    In:  Other Sources
    Details
    Publication Date: 2018-12-01
    Description: Solar thermonuclear process, radiation phenomena, structural measurements, observations and properties
    Keywords: SPACE SCIENCES
    Format: text
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  • 18
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    Mission and Design of an Orbiting Radio Astronomy Explorer (1964)
    In:  CASI
    Details
    Publication Date: 2019-05-23
    Description: Radio Astronomy Explorer /RAE/ satellite for measuring intensity of radio signals from celestial sources
    Keywords: SPACE SCIENCES
    Type: NASA-TM-X-51971
    Format: application/pdf
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  • 19
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    Satellite observations of type 3 solar radio bursts at low frequencies (1973)
    In:  CASI
    Details
    Publication Date: 2019-06-27
    Description: Type III solar radio bursts were observed from 10 MHz to 10 KHz by satellite experiments above the terrestrial plasmasphere. Solar radio emission in this frequency range results from excitation of the interplanetary plasma by energetic particles propagating outward along open field lines over distances from 5 solar radii to at least 1 AU from the sun. This review summarizes the morphology, characteristics and analysis of individual as well as storms of bursts. Burst rise times are interpreted in terms of exciter length and dispersion while decay times refer to the radiation damping process. The combination of radio observations at the lower frequencies and in-situ measurements on nonrelativistic electrons at 1 AU provide data on the energy range and efficiency of the wave-particle interactions responsible for the radio emission.
    Keywords: SPACE SCIENCES
    Type: NASA-TM-X-70540 , X-693-73-346
    Format: application/pdf
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  • 20
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    Asteroid selection for mission opportunities (1972)
    In:  CASI
    Details
    Publication Date: 2019-06-27
    Description: A study to assess the present state of knowledge of asteroids as well as the rate of change of that knowledge to better identify the mission and target priorities for advanced planning of asteroidal flights in the 1980's is presented. Topics discussed include; the present state of asteroid knowledge, the scientific goals and priorities attached to asteroid exploration, the anticipated advances in knowledge over the current decade, asteroid mission consideration, and asteroid selection. Data sheets for 118 asteroids are contained. These are asteroids for which some data is available over and above orbital parameters and magnitude.
    Keywords: SPACE SCIENCES
    Type: NASA-CR-129247 , P-42
    Format: application/pdf
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