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Workspace Method MagFieldsCalcExpand1D


Interpolation of 1D raw atmospheric fields to create 2D or 3D
homogeneous magnetic fields.  Derived from AtmFieldsCalcExpand1D

The method works as MagFieldsCalc, but accepts only raw 1D
magnetic fields. The raw data is interpolated to p_grid and
the obtained values are applied for all latitudes, and also
longitudes for 3D, to create a homogeneous atmosphere.

Authors: Richard Larsson


MagFieldsCalcExpand1D( mag_u_field, mag_v_field, mag_w_field, p_grid, lat_grid, lon_grid, mag_u_field_raw, mag_v_field_raw, mag_w_field_raw, atmosphere_dim, interp_order )


OUTmag_u_field(Tensor3)Zonal component of the magnetic field.
OUTmag_v_field(Tensor3)Meridional component of the magnetic field.
OUTmag_w_field(Tensor3)Vertical component of the magnetic field.
INp_grid(Vector)The pressure grid.
INlat_grid(Vector)The latitude grid.
INlon_grid(Vector)The longitude grid.
INmag_u_field_raw(GriddedField3)Raw zonal component of the magnetic field.
INmag_v_field_raw(GriddedField3)Raw meridional component of the magnetic field.
INmag_w_field_raw(GriddedField3)Raw vertical component of the magnetic field.
INatmosphere_dim(Index)The atmospheric dimensionality (1-3).
GINinterp_order(Index, Default: 1)Interpolation order (1=linear interpolation).