Search Results - "Del Zanna, G."
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CHIANTI—An Atomic Database for Emission Lines. XVI. Version 10, Further Extensions
Published in The Astrophysical journal (01-03-2021)“…Abstract We present version 10 of the CHIANTI package. In this release, we provide updated atomic models for several helium-like ions and for all the ions of…”
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Modelling stellar irradiances I: the transition regions of FGKM stars
Published in Monthly notices of the Royal Astronomical Society (01-11-2024)“…ABSTRACT We employed advanced ionization equilibrium models that we developed in Dufresne et al. (2024), which include charge transfer and density effects, to…”
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CHIANTI—AN ATOMIC DATABASE FOR EMISSION LINES. XIII. SOFT X-RAY IMPROVEMENTS AND OTHER CHANGES
Published in The Astrophysical journal (01-02-2013)“…The CHIANTI spectral code consists of two parts: an atomic database and a suite of computer programs in Python and IDL. Together, they allow the calculation of…”
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CHIANTI—An Atomic Database for Emission Lines. XVII. Version 10.1: Revised Ionization and Recombination Rates and Other Updates
Published in The Astrophysical journal. Supplement series (01-10-2023)“…Abstract The CHIANTI atomic database provides sets of assessed data that are used for simulating spectral observations of astrophysical plasmas. This article…”
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Helium line emissivities for nebular astrophysics
Published in Monthly notices of the Royal Astronomical Society (28-04-2022)“…ABSTRACT We present the results of several collisional-radiative models describing optically thin emissivities of the main lines in neutral helium formed by…”
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Satellite lines from auto-ionizing states of Fe xvi and the problems with the X-ray Fe xvii lines
Published in Monthly notices of the Royal Astronomical Society (01-07-2024)“…ABSTRACT We present new calculations of atomic data needed to model auto-ionizing states of Fe xvi. We compare the state energies, radiative and excitation…”
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SIMULTANEOUS IRIS AND HINODE/EIS OBSERVATIONS AND MODELING OF THE 2014 OCTOBER 27 X2.0 CLASS FLARE
Published in The Astrophysical journal (10-01-2016)“…ABSTRACT We present a study of the X2-class flare which occurred on 2014 October 27 and was observed with the Interface Region Imaging Spectrograph (IRIS) and…”
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JOINT HIGH TEMPERATURE OBSERVATION OF A SMALL C6.5 SOLAR FLARE WITH IRIS/EIS/AIA
Published in The Astrophysical journal (20-04-2015)“…ABSTRACT We present the observation of a C6.5 class flare on 2014 February 3, obtained with the Interface Region Imaging Spectrograph (IRIS) and the EUV…”
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CHIANTI—An Atomic Database for Emission Lines—Paper. XVIII. Version 11, Advanced Ionization Equilibrium Models: Density and Charge Transfer Effects
Published in The Astrophysical journal (01-10-2024)“…Abstract Version 11 of the chianti database and software package is presented. Advanced ionization equilibrium models have been added for low charge states of…”
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Chorus wave power at the strong diffusion limit overcomes electron losses due to strong diffusion
Published in Nature communications (27-02-2024)“…Earth’s radiation belts consist of high-energy charged particles trapped by Earth’s magnetic field. Strong pitch angle diffusion of electrons caused by…”
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Multiwavelength Observations by XSM, Hinode, and SDO of an Active Region. Chemical Abundances and Temperatures
Published in The Astrophysical journal (01-08-2022)“…Abstract We have reviewed the first year of observations of the Solar X-ray Monitor (XSM) on board Chandrayaan-2 and the available multiwavelength observations…”
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Coronal Diagnostics from Narrowband Images Around 30.4 nm
Published in Solar physics (01-07-2012)“…Images taken in the band centered at 30.4 nm are routinely used to map the radiance of the He ii Ly α line on the solar disk. That line is one of the…”
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On the validity of the ICFT R-matrix method: Fe xiv
Published in Monthly notices of the Royal Astronomical Society (11-12-2015)“…Recently, Aggarwal & Keenan published a Dirac R-matrix (darc) calculation for the electron-impact excitation of Fe xiv. A 136-level…”
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Advancing Solar and Heliospheric Science Through the Ongoing Development and Support of Atomic and Laboratory Plasma Physics
Published in Frontiers in astronomy and space sciences (19-01-2023)“…This paper outlines the necessity for the availability, accessibility, and expansion of atomic physics data and analysis tools for the meaningful…”
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A Multi-Wavelength Study of the Compact M1 Flare on October 22, 2002
Published in Solar physics (01-03-2006)“…In this paper we present a further study of the Ml class flare observed on October 22, 2002. We focus on the SOHO Coronal Diagnostic Spectrometer (CDS)…”
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A benchmark study of atomic models for the transition region against quiet Sun observations
Published in Monthly notices of the Royal Astronomical Society (01-05-2023)“…ABSTRACT The use of the coronal approximation to model line emission from the solar transition region has led to discrepancies with observations over many…”
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Effects of density on the oxygen ionization equilibrium in collisional plasmas
Published in Monthly notices of the Royal Astronomical Society (01-09-2020)“…ABSTRACT The ion populations most frequently adopted for diagnostics in collisional plasmas are derived from the density independent coronal approximation. In…”
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Modelling low charge ions in the solar atmosphere
Published in Monthly notices of the Royal Astronomical Society (01-08-2021)“…ABSTRACT Extensions have been made recently to the coronal approximation for the purpose of modelling line emission from carbon and oxygen in the lower solar…”
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New atomic data for C i Rydberg states compared with solar UV spectra
Published in Monthly notices of the Royal Astronomical Society (01-11-2023)“…ABSTRACT We use the Breit–Pauli R-matrix method to calculate accurate energies and radiative data for states in C i up to n = 30 and with l ≤ 3. We provide the…”
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Are Coronal Loops Isothermal or Multithermal?
Published in The Astrophysical journal (20-01-2009)“…Surprisingly few solar coronal loops have been observed simultaneously with TRACE and SOHO/Coronal Diagnostics Spectrometer (CDS), and even fewer analyses of…”
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