 The data file
        simulates the vibrational structure of the dispersed
        fluorescence spectrum obtained by exciting v2 = 1 in
        the A state of CFBr. (See Rotational
          Structure of the A-X electronic transition in CFBr for the rotational
        structure.) The data file is a reasonably straightforward
        example of simulating vibrational structure. Notes:
The data file
        simulates the vibrational structure of the dispersed
        fluorescence spectrum obtained by exciting v2 = 1 in
        the A state of CFBr. (See Rotational
          Structure of the A-X electronic transition in CFBr for the rotational
        structure.) The data file is a reasonably straightforward
        example of simulating vibrational structure. Notes:
      
        - The 79Br/81Br isotope splitting was
          not resolved in the dispersed fluorescence spectrum, so the
          set-up is for the average of the two.
- The x13
          and x23
          terms in the ground state must be included using perturbations.
- The vibrational mode displacements were determined by
          empirical fitting, so no information about the nuclei have
          been entered.
- A dispersed fluorescence rather than an absorption spectrum
          is simulated by setting Initial to
          false for the ground state manifold (X) and true for the upper
          state manifold (A).
      This file also provides an example of using a 
Non-Boltzmann Population to simulate
      fluorescence from v
2 = 1 rather than v
2 = 0
      that a Boltzmann population would imply. This was set up by:
      
        - Use "View","States"
          to bring up the State Details Window.
- Select the A state in the Active Object combo
          box at the top of the window.
- Right click on the required state in the "Eigenvalues" pane
          (the lower matrix), here state number 2 "0,1,0", and select
          "Add to population selection".
 
- The required population is now a parameter in the A state manifold object.
- To use the manually entered populations rather than a
          Boltzmann population, set the temperature negative.
Note that a similar effect can be obtained using vMin and vMax for various
        modes, though an implementation restriction in the current
        version means that values of vMin
        > 0 are likely to slow calculations for intensities
        considerably.
      Dispersed fluorescence spectrum from v
2 = 1:
      
     
    Dispersersed fluorescence spectrum from the origin band, obtained by
    setting T = 300: