Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....43..285l&link_type=abstract
Astronomy and Astrophysics, vol. 43, no. 2, Oct. 1975, p. 285-290.
Astronomy and Astrophysics
Astrophysics
19
Collision Parameters, Ground State, Iron, Particle Collisions, Proton Energy, Solar Corona, Atomic Excitations, Computer Programs, Coulomb Collisions, Electron States, Electron Transitions, Scattering Cross Sections, Solar Temperature
Scientific paper
Values of proton collisional cross-sections at coronal energies have been computer for all transitions between magnetic sublevels of the Fe(+12) and Fe(+13) ground configurations. Semiclassical Coulomb excitation theory was used with the resulting truncated Schroedinger equations being directly integrated. The corresponding rate constants for coronal temperatures are presented and comparison is made with previous results.
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