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Workspace Method propmat_clearskyAddOnTheFly

Description

Calculates gas absorption coefficients line-by-line.

This method can be used inside propmat_clearsky_agenda just like
propmat_clearskyAddFromLookup. It is a shortcut for putting in some
other methods explicitly, namely:

  1. AbsInputFromRteScalars
  2. Execute abs_xsec_agenda
  3. abs_coefCalcFromXsec
  4. propmat_clearskyAddFromAbsCoefPerSpecies

The calculation is for one specific atmospheric condition, i.e., a set
of pressure, temperature, and VMR values.

Authors: Stefan Buehler, Richard Larsson

Synopsis

propmat_clearskyAddOnTheFly( propmat_clearsky, nlte_source, dpropmat_clearsky_dx, dnlte_dx_source, nlte_dsource_dx, f_grid, abs_species, jacobian_quantities, rtp_pressure, rtp_temperature, rtp_nlte, rtp_vmr, abs_xsec_agenda )

Variables

OUT+INpropmat_clearsky(ArrayOfPropagationMatrix)This contains the absorption coefficients for one point in the atmosphere (one set of pressure, temperature, magnetic field, and VMR values).
OUT+INnlte_source(ArrayOfStokesVector)Variable to contain the additional source function due to NLTE effects.
OUT+INdpropmat_clearsky_dx(ArrayOfPropagationMatrix)Partial derivative of absorption coefficients.
OUT+INdnlte_dx_source(ArrayOfStokesVector)NLTE partial derivatives output is two parts: S*dB/dx+dS/dx*B.
OUT+INnlte_dsource_dx(ArrayOfStokesVector)NLTE partial derivatives output is two parts: S*dB/dx+dS/dx*B.
INf_grid(Vector)The frequency grid for monochromatic pencil beam calculations.
INabs_species(ArrayOfArrayOfSpeciesTag)Tag groups for gas absorption.
INjacobian_quantities(ArrayOfRetrievalQuantity)The retrieval quantities in the Jacobian matrix.
INrtp_pressure(Numeric)Pressure at a radiative transfer point.
INrtp_temperature(Numeric)Temperature at a radiative transfer point.
INrtp_nlte(EnergyLevelMap)NLTE temperature/ratio at a radiative transfer point.
INrtp_vmr(Vector)Absorption species abundances for radiative transfer calculations.
INabs_xsec_agenda(Agenda)Agenda to calculate scalar gas absorption cross sections.