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SOLAR AND THERMAL RADIATION IN JUPITERS ATMOSPHERE - INITIAL RESULTS OF THE GALILEO PROBE NET FLUX RADIOMETER

机译:朱庇特大气的太阳和热辐射-伽利略探针净通量辐射计的初始结果。

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The Galileo probe net flux radiometer measured radiation within Jupiter's atmosphere over the 125-kilometer altitude range between pressures of 0.44 bar and 14 bars. Evidence for the expected ammonia cloud was seen in solar and thermal channels down to 0.5 to 0.6 bar. Between 0.6 and 10 bars large thermal fluxes imply very low gaseous opacities and provide no evidence for a deep water cloud. Near 8 bars the water vapor abundance appears to be about 10 percent of what would be expected for a solar abundance of oxygen. Below 8 bars, measurements suggest an increasing water abundance with depth or a deep cloud layer. Ammonia appears to follow a significantly subsaturated profile above 3 bars. Unexpectedly high absorption of sunlight was found at wavelengths greater than 600 nanometers.
机译:伽利略探测器净通量辐射计测量了木星大气中在0.44 bar和14 bar压力之间的125公里海拔范围内的辐射。在太阳和热通道中,氨气浓度低至0.5至0.6 bar的证据都可以看到。在0.6到10巴之间,大的热通量意味着很低的气体混浊度,也没有提供深水云的证据。接近8巴时,水蒸气的丰度似乎约为太阳能中氧气的丰度的10%。低于8条,测量结果表明水的丰度随着深度或深层云层的增加而增加。氨似乎在3 bar以上遵循明显的亚饱和曲线。在波长大于600纳米的情况下,意外地吸收了很高的阳光。

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