Contents of this distribution:

Files:
  COPYING:          copyright terms (GPL license)
  InversionKit.jar: compiled program (can be run directly - see doc.pdf)
  Makefile:         a makefile which will replace InversionKit with a new
                    compiled version (this should be identical to previous
                    version if no changes are made to the source files)
  README:           this file
  doc.pdf:          a short manual which explains how to use InversionKit
  amde2famde.f:     a fortran program to convert a binary amde file to an
                    ASCII famde file which can be read by InversionKit

Folders:
  src:              contains java source files 
  classes:          contains java class files (files obtained after compilation)
                    including class files extracted from jlapack

!------------------------------------------------------------------------------
! List of changes:
!------------------------------------------------------------------------------
1.2:  - can now use full grid to calculate the different integrals (using a
        sliding window technique) which intervene in RLS and SOLA inversions.
        For the RLS inversions, this is supplemented by the use of b-splines
        which allow the use of a different grid for the output inverted
        functions.
      - corrected bug in which the inversion would sometimes update twice
        when changing the number of grid points in the inversion
      - averaging kernels are only calculated as needed so as to gain time when
        changing parameters such as Lambda, Delta of Theta

1.1:  - can read eigenfunction in FILOU format
      - can read .osc file from earlier versions of CESAM (i.e. before CESAM2k)
      - addition of separate field for IDL titles in plots so as to avoid
        difficulties with special characters
      - removed index array for rotation splittings and frequency shifts:
        - sort is very slightly slower
        - deleting rows is much faster
        - simpler code

1.0: First version to be distributed
!------------------------------------------------------------------------------
