The SUMER spectral atlas of solar-disk features

By W. Curdt, P. Brekke, U. Feldman, K. Wilhelm, B. Dwivedi, U. Schühle, P. Lemaire. 2001

282 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/d4ac7b9917cf065ea7d99e892b3cc3101be12a3e

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In Astronomy and Astrophysics

1. M. Haberreiter
2. J. C. Raymond
3. J. Harder
4. J. Fontenla
5. W. Curdt
6. Hai-Jun Tian
7. A. Bosman
8. Rudolf Loeser

Citations in the corpus

• Photodissociation and photoionisation of atoms and molecules of astrophysical interest (2017, methodology): “The solar ultraviolet flux is measured directly in the series of SOHO-SUMER observations (Curdt et al. 2001) for λ < 160 nm and also by the UARS SOLSTICE mission (Woods et al. 1996), including longer wavelengths.”
• Models of the Solar Chromosphere and Transition Region from SUMER and HRTS Observations: Formation of the Extreme-Ultraviolet Spectrum of Hydrogen, Carbon, and Oxygen (2008, background): “Figure 1 shows, in green for wavelengths 67Y147 nm, the SUMER atlas spectrum from the average quiet Sun at disk center from Curdt et al. (2001) and, in brown for wavelengths 147Y173 nm, the HRTS quiet-Sun spectrum from Brekke (1993a).”
• SEMIEMPIRICAL MODELS OF THE SOLAR ATMOSPHERE. III. SET OF NON-LTE MODELS FOR FAR-ULTRAVIOLET/EXTREME-ULTRAVIOLET IRRADIANCE COMPUTATION (2009, methodology): “Observations by the SOHO/SUMER instrument have been used to produce the atlas of Curdt et al. (2001) showing the spectrum of the average quiet-Sun in the wavelength range 700–1500 Å.”
• Semiempirical Models of the Solar Atmosphere. I. The Quiet- and Active Sun Photosphere at Moderate Resolution (2006, result): “Also, our calculations of the O i resonance lines at 1027.4 and 1028.5 8, formed in the chromosphere, are in better agreement with SUMER observations (Curdt et al. 2001) when the reduced abundance is used.”
• Elemental Abundances and Post-Coronal Mass Ejection Current Sheet in a Very Hot Active Region (2002, background): “While the relative intensities of Vernazza & Reeves (1978) agree quite well with the SUMER spectrum of Curdt et al. (2001) for the quiet Sun, the relative intensities vary by up to a factor of 2 between quiet and active regions.”