Proton collisional excitation in the ground configuration of Fe/11+/

Details Proton collisional excitation in the ground configuration of Fe/11+/ Proton collisional excitation in the ground configuration of Fe/11+/

Feb 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...220..366l&link_type=abstract

Astrophysical Journal, Part 1, vol. 220, Feb. 15, 1978, p. 366-369.

Astronomy and Astrophysics

Astrophysics

12

Ground State, Iron, Proton Scattering, Solar Corona, Transition Probabilities, Coulomb Potential, Electron Impact, Metal Ions, Particle Collisions, Schroedinger Equation, Solar Corpuscular Radiation

Scientific paper

Proton collisional excitation cross sections at solar coronal energies for the Fe(11+) /3S(2)3p(3)/ ground-configuration transitions are presented. Semiclassical Coulomb excitation theory is used with direct integration of the resulting Schroedinger equation. The rate constants at coronal temperatures are compared with the corresponding ones for electron impact excitation.

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