• DocumentCode
    770030
  • Title

    Thermal Radio Radiation from the Moon and Planets

  • Author

    Mayer, Cornell H.

  • Volume
    8
  • Issue
    3
  • fYear
    1964
  • fDate
    7/1/1964 12:00:00 AM
  • Firstpage
    236
  • Lastpage
    247
  • Abstract
    Thermal radio radiation has been observed from the moon, Mercury, Venus, Mars, Jupiter, and Saturn. The most important result of the observations is the discovery that the temperature at the surface of Venus, beneath the clouds, is greater than 600° K. The thermal radio radiation from the moon comes from beneath the surface and gives information about the temperature distribution and variation which can be interpreted in terms of the physical characteristics of the subsurface material. This also should apply to the planets with thin atmospheres. The thermal radio radiation from Jupiter should give information about the temperature distribution in the extensive absorbing atmosphere, but the intensity of the thermal radiation is confused by the nonthermal radiation of the radiation belts and cannot be accurately specified until more observational data are available.
  • Keywords
    Atmosphere; Belts; Clouds; Jupiter; Mars; Moon; Planets; Saturn; Temperature distribution; Venus;
  • fLanguage
    English
  • Journal_Title
    Military Electronics, IEEE Transactions on
  • Publisher
    ieee
  • ISSN
    0536-1559
  • Type

    jour

  • DOI
    10.1109/TME.1964.4323150
  • Filename
    4323150