Coronal hole boundary brightness in lambda 284 of Fe XV

Details Coronal hole boundary brightness in lambda 284 of Fe XV Coronal hole boundary brightness in lambda 284 of Fe XV

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979soph...62..343n&link_type=abstract

Solar Physics, vol. 62, June 1979, p. 343-346.

Physics

Brightness, Coronal Holes, Solar Spectra, Boundaries, Iron, Isophotes, Luminous Intensity

Scientific paper

An attempt is made to specify coronal hole boundaries in the brightness of λ284 of Fe XV. This is done by evaluating brightnesses of λ284 at boundaries selected by various groups. These results are in quite good agreement and suggest a brightness value of (0.8 ± 0.4) × 1012 photons cm-2 s-1 sr-1 for coronal hole boundaries in λ284. The examination of a number of isophote maps near this boundary brightness shows no consistent brightness gradient.

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