Formation of silicate and titanium clouds on hot Jupiters
We present the first application of a bin-scheme microphysical and vertical transport model to determine the size distribution of titanium and silicate cloud particles in the atmospheres of hot Jupiters. We predict particle size distributions from first principles for a grid of planets at four repre...
| Main Authors: | , , , |
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| Format: | Journal article |
| Published: |
American Astronomical Society
2018
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