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Workspace Method propmat_clearskyAddZeeman

Description

Calculates Zeeman-effected absorption coefficients.

This method will, for each Zeeman species, make a local
ArrayOfLineRecord for the various transition types with Zeeman
altered LineRecord(s).  These are then composed into a single
ArrayOfArrayOfLineRecord which is processed as per the scalar case.

The line broadened absorption coefficients are finally multiplied with
the transition type rotation matrix and the new variable is inserted into
the out variable. Only species containing a -Z- tag are treated.

Note that between 55 GHz and 65 GHz there is usually ~700 O_2 lines,
however, when this Zeeman splitting method is used, the number of
lines is increased to about 45,000. Be aware that this is a time
consuming method.

The 'manual_zeeman*' variables will let the user set their own simple
magnetic field.  This path can be accessed by setting
*manual_zeeman_tag* different from zero.  The user is also advided to
read the theory guide to understand what the different variables will
do in the Zeeman theory.  Note that angles are in degrees and strength
in Tesla.

Authors: Richard Larsson

Synopsis

Variables