G
G. Del Zanna
Researcher at University of Cambridge
Publications - 220
Citations - 11381
G. Del Zanna is an academic researcher from University of Cambridge. The author has contributed to research in topics: Coronal loop & Corona. The author has an hindex of 52, co-authored 202 publications receiving 10457 citations. Previous affiliations of G. Del Zanna include University College London & Lawrence Livermore National Laboratory.
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Chianti—an atomic database for emission lines. xiii. soft x-ray improvements and other changes
TL;DR: The CHIANTI spectral code as mentioned in this paper consists of two parts: an atomic database and a suite of computer programs in Python and IDL, together, they allow the calculation of the optically thin spectrum of astrophysical objects and provide spectroscopic plasma diagnostics for the analysis of the astrophysical spectra.
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CHIANTI - an atomic database for emission lines. IX. Ionization rates, recombination rates, ionization equilibria for the elements hydrogen through zinc and updated atomic data
TL;DR: The CHIANTI database as mentioned in this paper provides a set of atomic data for the interpretation of astrophysical spectra emitted by collisionally dominated, high temperature, optically thin sources.
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CHIANTI-An Atomic Database for Emission Lines. VII. New Data for X-Rays and Other Improvements
TL;DR: The CHIANTI atomic database as mentioned in this paper contains atomic energy levels, wavelengths, radiative transition probabilities, and collisional excitation data for a large number of ions of astrophysical interest.
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SDO/AIA response to coronal hole, quiet Sun, active region, and flare plasma
TL;DR: In this article, the authors examined the contribution of spectral lines and continuum emission to the EUV channels of the Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO) in different regions of the solar atmosphere.
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CHIANTI – An atomic database for emission lines. Version 8
TL;DR: This version of the CHIANTI database includes a large amount of new data and ions, which represent a significant improvement in the soft X-ray, EUV and UV spectral regions, which several space missions currently cover.