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) onHinode
The Astrophysical Journal Supplement Series2008Vol. 176(2), pp. 511–535
Citations Over TimeTop 1% of 2008 papers
Abstract
We present spectral line wavelengths, identifications, and intensities in the 171-211 and 245-291 Å ranges from five solar plasma regions recorded by the Extreme-Ultraviolet Imaging Spectrometer (EIS) on Hinode. The recorded data were emitted from a quiet region, two active areas on the solar disk, a limb region, and a region 20'' above the limb. The line list contains 500 lines of which 55% were identified with previously known transitions. Although the EIS spectral coverage is limited to two ranges approximately 40 Å wide, the identified lines belong to a total of 56 ions from 15 elements.
Related Papers
- → Design of a compact hyperspectral imaging spectrometer with a freeform surface based on anastigmatism(2020)20 cited
- Airborne Visible/Infrared Imaging Spectrometer (AVIRIS)(1988)
- → Analysis method of the Offner hyperspectral imaging spectrometer based on vector aberration theory(2020)23 cited
- → Airborne Visible/Infrared Imaging Spectrometer (Aviris) Spectrometer Design And Performance(1987)19 cited
- → Design and manufacture of compact long-slit spectrometer for hyperspectral remote sensing(2021)4 cited