Fig. 3 from Coronal Composition above the Solar Equator and the North Pole as Determined from Spectra Acquired by the SUMER Instrument on SOHO

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Coronal Composition above the Solar Equator and the North Pole as Determined from Spectra Acquired by the SUMER Instrument on SOHO

Authors: U. Feldman, U. Schühle, K. G. Widing, and J. M. Laming

Feldman et al. 1998 The Astrophysical Journal 505 999.

Provider: AAS Journals

Caption: Fig. 3.

Plot of the effective FIP bias as a function of temperature for the corona above the quiet equatorial region. (a) High‐FIP lines; and (b) low‐FIP lines. Li‐like Ne VIII, Na IX, and Mg X lines are not shown.

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