Configure the simple spectral model parameters Gas optics for simple spectral models are described as N triangles of ln(kappa) for each of M gases. Each triangle id defined by the absorption coefficient at central wavenumber, nu0 a central wavenumber nu0 the slope d ln(kappa)/d nu By default there are two gases (h2o and co2) (for the LW). h2o has three triangles (rotational lines, and a continuum with infinite slope) co2 has a single triangle Absorption coefficents are defined at pref and pressure-broadened as p/pref Spectral discretization is defined as max and min wavenumbers and a set of wavenumbers at which to evaluate absorption and Planck function If Tstar is provided the gas optics are for insolation
| Type | Intent | Optional | Attributes | Name | ||
|---|---|---|---|---|---|---|
| class(ty_optics_ssm), | intent(inout) | :: | this | |||
| character(len=32), | intent(in), | dimension(:) | :: | gas_names | ||
| real(kind=wp), | intent(in), | dimension(:,:) | :: | triangle_params | (ntriangles, 4) where the second dimension holds [gas_index, kappa0, nu0, l] |
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| real(kind=wp), | intent(in), | dimension(:) | :: | nus | Wavenumbers at which to evaluate Planck function and absorption coefficient |
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| real(kind=wp), | intent(in) | :: | nu_min | Upper and lower bounds of spectrum |
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| real(kind=wp), | intent(in) | :: | nu_max | Upper and lower bounds of spectrum |
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| real(kind=wp), | intent(in), | optional | :: | Tstar | Temperature for stellar insolation |
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| real(kind=wp), | intent(in), | optional | :: | tsi | Total solar irradiance |
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| real(kind=wp), | intent(in), | optional | :: | kappa_cld | ||
| real(kind=wp), | intent(in), | optional | :: | g_cld | ||
| real(kind=wp), | intent(in), | optional | :: | ssa_cld | cloud optical properties |
Empty if successful
| Type | Intent | Optional | Attributes | Name | ||
|---|---|---|---|---|---|---|
| class(ty_optics_ssm), | intent(inout) | :: | this | |||
| logical, | intent(in), | optional | :: | do_sw |