Jupiter's Deep Cloud Structure Revealed Using Keck Observations of Spectrally Resolved Line Shapes

@article{Bjoraker2015JupitersDC,
  title={Jupiter's Deep Cloud Structure Revealed Using Keck Observations of Spectrally Resolved Line Shapes},
  author={G. Bjoraker and M. Wong and I. Pater and M. 'Ad'amkovics},
  journal={arXiv: Earth and Planetary Astrophysics},
  year={2015}
}
Technique: We present a method to determine the pressure at which significant cloud opacity is present between 2 and 6 bars on Jupiter. We use: a) the strength of a Fraunhofer absorption line in a zone to determine the ratio of reflected sunlight to thermal emission, and b) pressure-broadened line profiles of deuterated methane (CH3D) at 4.66 microns to determine the location of clouds. We use radiative transfer models to constrain the altitude region of both the solar and thermal components of… Expand

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