James O Hornkohl1, Christian G Parigger, László Nemes
1The University of Tennessee Space Institute, 411 B. H. Goethert Parkway, Tullahoma, Tennessee 37388, USA. jhornkoh@utsi.edu
A novel computational method simplifies calculating diatomic rotational line strengths (Hönl-London factors) by directly determining them alongside line positions and parities for various molecules and n-photon spectra.
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