... | @@ -59,7 +59,7 @@ Copy and edit the file _inputs/example.nml_, rename it _corot-4b.nml_. An extend |
... | @@ -59,7 +59,7 @@ Copy and edit the file _inputs/example.nml_, rename it _corot-4b.nml_. An extend |
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light_source_radius = 814e6 ! (m) radius of the light source
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light_source_radius = 814e6 ! (m) radius of the light source
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light_source_range = 13.5e9 ! (m) distance between the target and the light source
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light_source_range = 13.5e9 ! (m) distance between the target and the light source
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light_source_effective_temperature = 6190 ! (K) light source effective temperature
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light_source_effective_temperature = 6190 ! (K) light source effective temperature
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```text
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```
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5. As a starting point, we will use a metallicity of 1 times the solar metallicity, no cloud, and a fixed eddy diffusion coefficient. Because of the effective temperature of the planet, TiO, VO and FeH are unlikely to have significant absorptions, so we will remove them in order to speed-up the calculations:
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5. As a starting point, we will use a metallicity of 1 times the solar metallicity, no cloud, and a fixed eddy diffusion coefficient. Because of the effective temperature of the planet, TiO, VO and FeH are unlikely to have significant absorptions, so we will remove them in order to speed-up the calculations:
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```text
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```text
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metallicity = 1.0 ! (solar metallicity) atmospheric metallicity
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metallicity = 1.0 ! (solar metallicity) atmospheric metallicity
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