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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. 1.

EIT image of the 1 × 106 K solar corona taken at 171 Å. Transitions of Fe IX and Fe X are the most prominent contributors to the detected emission.

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