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B. C. Monsignori Fossi
Researcher at Arcetri Astrophysical Observatory
Publications - 23
Citations - 2439
B. C. Monsignori Fossi is an academic researcher from Arcetri Astrophysical Observatory. The author has contributed to research in topics: Solar flare & Coronal mass ejection. The author has an hindex of 10, co-authored 23 publications receiving 2302 citations.
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Journal ArticleDOI
CHIANTI - an atomic database for emission lines - I. Wavelengths greater than 50 Å
TL;DR: The CHIANTI database as mentioned in this paper is a set of atomic data and transition probabilities necessary to calculate the emission line spectrum of astrophysical plasmas, including atomic energy levels, atomic radiative data such as wavelengths, weighted oscillator strengths and A values, and electron collisional excitation rates.
Journal ArticleDOI
Spectroscopic diagnostics in the VUV for solar and stellar plasmas
Abstract: The VUV emission spectra from the solar atmosphere and stellar atmospheres have been intensively studied during the past 25 years with several major space programs In this review we discuss the spectroscopic diagnostic techniques used to study astrophysical plasmas, the atomic processes involved, the recent observations and the plans for future space missions
Book ChapterDOI
The X-UV spectrum of thin plasmas
TL;DR: Le spectre du rayonnement emis par un plasma optiquement mince et chaud (10 4 -10 8 K) determine numeriquement dans la bande spectrale 1-2000 A est presente as mentioned in this paper.
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Models for inner corona parameters
TL;DR: In this article, the authors evaluate the differential emission measure distribution from the observational data and discuss the methods to evaluate differential emission measurement distribution from XUV line radiation from the sun. But the authors focus on the structure of the inner corona.
Journal ArticleDOI
The Xray-EUV spectrum of optically thin plasmas
TL;DR: In this paper, the Xray-EUV spectral code for optically thin plasmas has been updated with more accurate atomic data computations, and several lines have been added.