Observation of possible Fe XVII 2p5 3p/1S0/ - 2p5 3s/1P1, 3P1/ transitions in spectra of a solar active region and flare

Details Observation of possible Fe XVII 2p5 3p/1S0/ - 2p5 3s/1P1, 3P1/ transitions in spectra of a solar active region and flare Observation of possible Fe XVII 2p5 3p/1S0/ - 2p5 3s/1P1, 3P1/ transitions in spectra of a solar active region and flare

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...43..111k&link_type=abstract

Solar Physics, vol. 43, July 1975, p. 111-115.

Physics

5

Electron Transitions, Iron, Line Spectra, Solar Flares, Solar Spectra, Atomic Spectra, Electronic Spectra, Oso-7, Solar Activity, Transition Probabilities

Scientific paper

Expected wavelengths and relative intensities are obtained from previous calculations for the hitherto unobserved transitions 2p5 3p(1SO) - 2p5 3s(1P1, 3P1) in Fe XVII. A candidate pair of lines at 197.05 A and 242.09 A was found in laboratory spectra and appears to be present in the spectra of a solar active region observed by the OSO-7 Goddard spectroheliograph as well as in the spectrum of a Skylab-observed solar flare.

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