Atomic Parameters for Fe XVIII Derived From Solar Coronal Line Emission.

Details Atomic Parameters for Fe XVIII Derived From Solar Coronal Line Emission. Atomic Parameters for Fe XVIII Derived From Solar Coronal Line Emission.

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976baas....8..523r&link_type=gif

Bulletin of the American Astronomical Society, Vol. 8, p.523

Astronomy and Astrophysics

Astronomy

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