activity
20082025
most citedCHIANTI -- an atomic database for emission lines -- Paper XVI: Version 10, further extensions

385 citations · 783 across the 20 of their papers we have counts for

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12 papers · 1 filter

astro-ph.SR2025★ 6 cited

Reduced atomic models for large-scale computations: Fe XIII near-infrared lines

Giulio Del Zanna, Supriya Hebbur Dayananda

Accurate atomic models for astrophysical plasma can be very complex, requiring thousands of states. However, for a variety of applications such as large-scale forward models of the…

astro-ph.SR2024

Modelling Stellar Irradiances I: the transition regions of FGKM stars

Evangelia Deliporanidou, Giulio Del Zanna

We employed advanced ionisation equilibrium models that we developed in Dufresne et. al. (2024), which include charge transfer and density effects, to model UV stellar irradiances…

astro-ph.SR2022★ 14 cited

Soft X-ray Spectral Diagnostics of Multi-thermal Plasma in Solar Flares with Chandrayaan-2 XSM

N. P. S. Mithun, Santosh V. Vadawale, Giulio Del Zanna +7

Spectroscopic observations in X-ray wavelengths provide excellent diagnostics of the temperature distribution in solar flare plasma. The Solar X-ray Monitor (XSM) onboard the Chand…

astro-ph.SR2022★ 13 cited

The Center-to-Limb Variation of Non-Thermal Velocities using IRIS Si IV

Yamini K. Rao, Giulio Del Zanna, Helen E. Mason

We study the non-thermal velocities in the quiet-sun using various high spatial, temporal, and spectral resolution observations from the Interface Region Imaging Spectrograph (IRIS…

astro-ph.SR2020

Study of the spatial association between an active region jet and a nonthermal type~ radio burst

Sargam M. Mulay, Rohit Sharma, Gherardo Valori +4

We aim to investigate the spatial location of the source of an active region (AR) jet and its relation with associated nonthermal type~III radio emission. An emission measure (EM)…

astro-ph.SR2019★ 20 cited

Hinode EIS line widths in the quiet corona up to 1.5 Rsun

G. Del Zanna, G. R. Gupta, H. E. Mason

We present an analysis of several Hinode EIS observations of coronal line widths in the quiet Sun, up to 1.5 Rsun radial distances. No significant variations are found, which indic…