Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007phrva..75b2709h&link_type=abstract
Physical Review A, vol. 75, Issue 2, id. 022709
Astronomy and Astrophysics
Astrophysics
6
Atomic Excitation And Ionization By Electron Impact, Abundances, Chemical Composition
Scientific paper
Experimental cross sections are reported for the Fe13+ coronal green line transition 3s23pP1/2o2-3s23pP3/2o2 at λ5303Å(2.338eV) . The center-of-mass interaction energies are in the range 1.7eV (below threshold) through threshold, to 6.6eV ( 2.9× threshold). Data are compared with results of a 135-level Breit-Pauli R -matrix theory. Present experiment detects a strong maximum in the excitation cross section of magnitude 15×10-16cm2 at 2.6eV . Smaller structures are observed between 3eV and 6.6eV , with a maximum cross section never exceeding about 1.2×10-16cm2 . All features are due to enhancement of the direct excitation via a multitude of narrow, closely-spaced resonances calculated by the theory, the effects of which are convoluted by the 125meV energy resolution of the present experiment. Iron is present in practically every astrophysical object, as well as being an impurity in fusion plasmas. Present results are the highest charge state in any ion for which an absolute excitation cross section has been measured.
Chutjian Ara
Hossain Sabbir
Raymond John C.
Smith Stephen J.
Tayal Swaraj S.
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