CH4 mixing ratios at microbar pressure levels of Jupiter as constrained by 3-micron ISO data
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文摘

Updated radiative transfer programs to construct a 3-mm emission model of CH4.

Compared the model with 3-mm ISO data of Jupiter to derive microbar CH4 mixing ratios.

Found at least 10 times smaller than CH4 mixing ratios from Galileo probe analysis.

Provided discussions on the photochemistry and vertical transport in the stratosphere.

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