CHIANTI—AN ATOMIC DATABASE FOR EMISSION LINES. XIII. SOFT X-RAY IMPROVEMENTS AND OTHER CHANGES

By E. Landi, Peter R. Young, K. Dere, G. D. Zanna, Helen E. Mason. 2013

400 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Mechanics of Materials

View Paper: https://www.semanticscholar.org/paper/b02ca3d59baad58b7dcce8d4c7e7fedcb419cc56

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Citations in the corpus

ALFVÉN WAVE SOLAR MODEL (AWSoM): CORONAL HEATING (2013, methodology): “The optically thin radiative energy loss in the lower corona is given by Qrad = NeNhΛ(Te), (6) where Nh is the hydrogen number density and Λ(Te) is the radiative cooling curve taken from the CHIANTI version 7.1 database (Landi et al. 2013a).”
CHIANTI - An atomic database for Emission Lines. Version 8 (2015, background): “These new collision strengths replace those in the 7.1 version of the CHIANTI database (Landi et al. 2013).”
A UNIFIED COMPUTATIONAL MODEL FOR SOLAR AND STELLAR FLARES (2015, methodology): “We model the radiative transfer in these regions using a radiative loss function which is obtained by summing all transitions in the CHIANTI database (Dere et al. 1997; Landi et al. 2013) except those already accounted for in Tables 1 and 2.”
The SAMI Galaxy Survey: shocks and outflows in a normal star-forming galaxy (2014, methodology): “We adopt the CHIANTI package written in IDL (Dere et al. 1997; Landi et al. 2013) to convert the flux ratios [S II] λ6716/[S II] λ6731 to electron densities assuming an electron temperature, Te, of 104 K.”
THERMAL DIAGNOSTICS WITH THE ATMOSPHERIC IMAGING ASSEMBLY ON BOARD THE SOLAR DYNAMICS OBSERVATORY: A VALIDATED METHOD FOR DIFFERENTIAL EMISSION MEASURE INVERSIONS (2015, methodology): “Figure 1 shows temperature response functions for the AIA EUV channels as computed by the Solarsoft routine aia_get_response(/temp,/evenorm,/chiantifix) using the CHIANTI 7.1.3 package (Landi et al. 2013).”
The multi-thermal emission in solar active regions (2013, methodology): “The latest v.7.1 CHIANTI ionization equilibrium tables (Landi et al. 2013) are adopted here.”