The Self-Consistent Field with Exchange for the Ground State and First Excited State of Fe ⁺¹³

Abstract

Results of self-consistent field calculations with exchange for the ground state (3 s ) ² (3 p ) and the first excited state (3 s ) (3 p ) ² of Fe ⁺¹³ are presented. The differences between energy levels of the terms are given, including the separation due to spin-orbit interaction. Integrals are given for use in the calculation of transition probabilities for lines of importance in the solar corona.