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Combination Difference Fitting

Observations containing an upper or lower level in common can be combined into a single observation corresponding to the difference in energy between the two levels in the other state. Fitting in this way can be helpful if one of the states is perturbed or unassigned. If using the linelist window fitting using this mode can be invoked from the "More" menu (rather than using the fit button). When fitting in this way the observations are internally sorted by upper or lower state as appropriate, and the resulting list is then scanned, combing observations where possible. Any observations that cannot be combined are discarded.

For more control, put the observations in a separate file, rather than using the linelist window, and is then probably easiest to work with using directives in the input file as shown below, though CDlower or CDupper can be selected as the default mode for a file in the log window. It is also possible to manually construct the appropriate equivalent transitions within the state of interest, even if they do not correspond to allowed transitions; PGOPHER does not require fitted transitions to be allowed.

CDupper/CDlower

The CDupper or CDlower directive can be used for observations that are already sorted so that those with common levels are adjacent. The directive applies to all following observations until a directive changes the observation type. For example, using lines in branch format, the pair of observations input as follows:
CDlower
P(6) 992.1870 1
R(4) 1012.0070 1
will be transformed into a single observation of 1012.0070-992.1870 = 19.82 corresponding to the difference between J" = 6 and J" = 4 in the lower state. Any observations that cannot be combined causes an error.

AutoCDupper/AutoCDlower

If the observations are not sorted the AutoCDupper or AutoCDlower directives can be used to automatically sort the observations before looking for common differences. In this mode a CDstart directive marks the start of the observations to be considered for conversion to combination differences, and the conversion happens when the AutoCDupper or AutoCDlower is encountered in the file. There is an implicit CDstart directive before the first observation, and after any observation type directive. The AutoCDupper or AutoCDlower directive can be followed by a flag that controls the handling of observations that are not part of an upper state combination difference:
This mode offers less control than the CDupper or CDlower directives as the mapping between the observations input and those actually fit can be less direct.. For example, any duplicate observations (those with identical upper and lower states) are combined into a single observation before looking for combination differences.

The following shows an example appropriate for a linear molecule:

CDstart
Excited 8 e 1 Ground 7 e 1 3035.9776 1 R(7) : Excited v=1 8 e - Ground v=0 7 e
Excited 8 e 1 Ground 8 e 1 2871.5452 1 Q(8) : Excited v=1 8 f - Ground v=0 8 e
Excited 9 e 1 Ground 8 e 1 3052.5730 1 R(8) : Excited v=1 9 e - Ground v=0 8 e
Excited 9 e 1 Ground 10 e 1 2663.1901 1 P(10) : Excited v=1 9 e - Ground v=0 10 e
Excited 10 e 1 Ground 10 e 1 2863.9385 1 Q(10) : Excited v=1 10 f - Ground v=0 10 e
Excited 11 e 1 Ground 10 e 1 3084.2618 1 R(10) : Excited v=1 11 e - Ground v=0 10 e
AutoCDupper include
Notes:

Estimated errors and correlations in the observations

When two observations are combined, the estimated standard deviation of the observation is derived from the standard deviations of the two observations, using standard error propagation methods. For two observations with standard deviation 1, the standard deviation of the difference will be sqrt(2). If three observations are combined in to two common differences, as for P(10), Q(10) and R(10) in the example above, then the correlation between the observations must be considered to obtain the correct statistical analysis. See J. Tellinghuisen, J. Molec. Spectrosc. 221, 244 (2003) for a discussion of this point. (Note this paper also points out that only two differences should be used for fitting in this case; including the third difference will also produced incorrect statistics.)

Overall example

The sample input file below shows how several of these possibilities can be combined in a single file. The data has been generated for a simple linear molecule, using the parameters given in the paper mentioned above.
# Normal lines
Line
Excited 5 e 1 Ground 5 e 1 2879.9890 1 Q(5) : Excited v=1 5 f - Ground v=0 5 e
Excited 9 e 1 Ground 9 e 1 2867.9519 1 Q(9) : Excited v=1 9 f - Ground v=0 9 e

# Explicit common differences in correct order
CDupper # Applies to following lines, which reduce to three observations
Excited 1 e 1 Ground 2 e 1 2844.2656 1 P(2) : Excited v=1 1 e - Ground v=0 2 e
Excited 2 e 1 Ground 2 e 1 2884.8006 1 Q(2) : Excited v=1 2 f - Ground v=0 2 e
Excited 3 e 1 Ground 2 e 1 2945.5659 1 R(2) : Excited v=1 3 e - Ground v=0 2 e

Excited 8 e 1 Ground 9 e 1 2686.9224 1 P(9) : Excited v=1 8 e - Ground v=0 9 e
Excited 10 e 1 Ground 9 e 1 3068.6981 1 R(9) : Excited v=1 10 e - Ground v=0 9 e

CDlower # Applies to following lines, which reduce to four observations
Excited 4 e 1 Ground 3 e 1 2964.5797 1 R(3) : Excited v=1 4 e - Ground v=0 3 e
Excited 4 e 1 Ground 4 e 1 2881.9914 1 Q(4) : Excited v=1 4 f - Ground v=0 4 e
Excited 4 e 1 Ground 5 e 1 2778.8584 1 P(5) : Excited v=1 4 e - Ground v=0 5 e

Excited 7 e 1 Ground 6 e 1 3018.8444 1 R(6) : Excited v=1 7 e - Ground v=0 6 e
Excited 7 e 1 Ground 8 e 1 2710.3938 1 P(8) : Excited v=1 7 e - Ground v=0 8 e
Excited 7 e 1 Ground 7 e 1 2874.7888 1 Q(7) : Excited v=1 7 f - Ground v=0 7 e

# Automatic common differences
CDstart # Start of block
# Note first line not a common difference
Excited 1 e 1 Ground 1 e 1 2885.6067 1 Q(1) : Excited v=1 1 f - Ground v=0 1 e
Excited 2 e 1 Ground 1 e 1 2926.1472 1 R(1) : Excited v=1 2 e - Ground v=0 1 e
Excited 2 e 1 Ground 3 e 1 2822.8136 1 P(3) : Excited v=1 2 e - Ground v=0 3 e
Excited 3 e 1 Ground 3 e 1 2883.5772 1 Q(3) : Excited v=1 3 f - Ground v=0 3 e
Excited 3 e 1 Ground 4 e 1 2801.0182 1 P(4) : Excited v=1 3 e - Ground v=0 4 e
Excited 5 e 1 Ground 4 e 1 2983.1304 1 R(4) : Excited v=1 5 e - Ground v=0 4 e
Excited 6 e 1 Ground 5 e 1 3001.2369 1 R(5) : Excited v=1 6 e - Ground v=0 5 e
Excited 5 e 1 Ground 6 e 1 2756.3627 1 P(6) : Excited v=1 5 e - Ground v=0 6 e
Excited 6 e 1 Ground 6 e 1 2877.5749 1 Q(6) : Excited v=1 6 f - Ground v=0 6 e
Excited 6 e 1 Ground 7 e 1 2733.5398 1 P(7) : Excited v=1 6 e - Ground v=0 7 e
AutoCDlower ignore # Applies to preceding lines; implicit block start

CDstart # Optional here, as preceding AutoCDlower forced block start
# Note first line not a common difference
Excited 8 e 1 Ground 7 e 1 3035.9776 1 R(7) : Excited v=1 8 e - Ground v=0 7 e
Excited 8 e 1 Ground 8 e 1 2871.5452 1 Q(8) : Excited v=1 8 f - Ground v=0 8 e
Excited 9 e 1 Ground 8 e 1 3052.5730 1 R(8) : Excited v=1 9 e - Ground v=0 8 e
Excited 9 e 1 Ground 10 e 1 2663.1901 1 P(10) : Excited v=1 9 e - Ground v=0 10 e
Excited 10 e 1 Ground 10 e 1 2863.9385 1 Q(10) : Excited v=1 10 f - Ground v=0 10 e
Excited 11 e 1 Ground 10 e 1 3084.2618 1 R(10) : Excited v=1 11 e - Ground v=0 10 e
Excited 10 e 1 Ground 11 e 1 2639.1611 1 P(11) : Excited v=1 10 e - Ground v=0 11 e
Excited 11 e 1 Ground 11 e 1 2859.4863 1 Q(11) : Excited v=1 11 f - Ground v=0 11 e
Excited 12 e 1 Ground 11 e 1 3099.2950 1 R(11) : Excited v=1 12 e - Ground v=0 11 e
AutoCDupper include

Line
Excited 1 e 1 Ground 0 e 1 2906.2757 1 R(0) : Excited v=1 1 e - Ground v=0 0 e