来自月球和行星的热无线电辐射

C. H. Mayer
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引用次数: 7

摘要

从月球、水星、金星、火星、木星和土星观测到热无线电辐射。观测的最重要的结果是发现金星表面云层下的温度大于600°k。来自月球的热无线电辐射来自地表下,提供了关于温度分布和变化的信息,这些信息可以根据地下物质的物理特性来解释。这也适用于大气层稀薄的行星。来自木星的热无线电辐射应该提供有关广泛吸收的大气中的温度分布的信息,但是热辐射的强度被辐射带的非热辐射所混淆,在获得更多观测数据之前无法精确指定。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Thermal Radio Radiation from the Moon and Planets
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.
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