Wavelengths and Intensities of Spectral Lines in the 171-211 and 245-291 Å Ranges from Five Solar Regions Recorded by the Extreme-Ultraviolet Imaging Spectrometer (EIS) on Hinode

By C. M. Brown, U. Feldman, J. Seely, C. Korendyke, H. Hara. 2008

137 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/b782b48cfeff77ef4568284a55af166c1886c191

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In Astronomy and Astrophysics

1. L. Green
2. A. Wallace
3. Peter R. Young
4. Hirohisa Hara
5. Tetsuya Watanabe
6. B. Kliem
7. J. Mariska
8. G. Aulanier

Citations in the corpus

• Photospheric flux cancellation and associated flux rope formation and eruption (2010, methodology): “The non-thermal velocities are calculated using the IDL Solar Software routineeis width2velocity which removes instrumental width, taken to be 0.057 Å for the 1′′ slit Brown et al. (2008), and thermal Doppler width.”
• High-precision density measurements in the solar corona I. Analysis methods and results for Fe XII and Fe XIII (2008, background): “We also note that Brown et al. (2008) list a Nixiv line as possibly blending with Sxi λ188.”