Tables of width cross-sections are presented for the broadening of general s-p and p-s atomic transitions by collisions with neutral atomic hydrogen. The transitions are characterized by the effective principal quantum numbers of the s and p states. Each cross-section is given for a relative velocity of 104 m s –1 together with an exponent α calculated on the assumption that the cross-section varies with velocity as v-α. The cross-sections were calculated using the methods described by the authors in a previous paper. The cross-sections are tested by using them in the synthesis of a selection of strong solar lines of sodium, calcium and iron with well-determined f-values. The abundances derived from the strong lines are consistent with the meteoritic values.
No takes yet. Share an insight, caveat, or question.
Anstee et al. (1995) studied this question.
Synapse has enriched 5 related papers. Consider them for comparative context: