Chianti-an atomic database for euv emission lines

By E. Landi. 2000

233 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/1d483c5019603d26854787457e6587c3c9b972ed

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

1. A. Vourlidas
2. M. Temmer
3. A. Thernisien
4. Jon A. Linker
5. C. Eyles
6. Roberto Lionello
7. J. Lemen
8. Z. Mikić

Citations in the corpus

• Global MHD Modeling of the Solar Corona and Inner Heliosphere for the Whole Heliosphere Interval (2008, methodology): “Simulated emission images were computed using the CHIANTI database (Dere et al., 1997).”
• Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) (2000, methodology): “We take typical differential emission measure distributions (DEMs) reported in the literature, predict the resulting solar spectral line emission using the CHIANTI software (Dere et al. 1997; Young et al. 2003), and combine the result with our calibration data.”