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pro vyhledávání: '"Landi E."'
Autor:
Dufresne, R. P., Del Zanna, G., Young, P. R., Dere, K. P., Deliporanidou, E., Barnes, W. T., Landi, E.
Version 11 of the CHIANTI database and software package is presented. Advanced ionization equilibrium models have been added for low charge states of seven elements (C, N, O, Ne, Mg, Si and S), and represent a significant improvement especially when
Externí odkaz:
http://arxiv.org/abs/2403.16922
Autor:
Landi, E, Schironi, F
Ancient astronomers faced the problem of dealing with arcs and angles in their observations and predictions without the help of modern trigonometry. The usual method to deal with such problems was the Menelaus Theorem, explicitly discussed and extens
Externí odkaz:
http://arxiv.org/abs/2310.09215
Autor:
Maggetti, C., Pinelli, D., Girometti, E., Papa, E., Medri, V., Landi, E., Avolio, F., Frascari, D.
Publikováno v:
In Chemosphere November 2024 367
Autor:
Cardenas-O'Toole, A., Landi, E.
In the present work we utilize ACE/SWICS in-situ measurements of the properties of the solar wind outside ICMEs in order to determine whether, and to what extent are the solar wind properties affected by the solar cycle. We focus on proton temperatur
Externí odkaz:
http://arxiv.org/abs/2201.05535
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 the beryllium, carbon and magnesium isoelectronic sequences that are abundant in astrophysical plasma
Externí odkaz:
http://arxiv.org/abs/2011.05211
The present work illustrates the potential of a new diagnostic technique that allows the measurement of the coronal magnetic field strength in solar active regions utilizing a handful of bright \ion[Fe x] and \ion[Fe xi] lines commonly observed by th
Externí odkaz:
http://arxiv.org/abs/2008.03532
Akademický článek
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Publikováno v:
In Chemical Engineering Research and Design March 2023 191:568-577
Akademický článek
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We present first results of a novel technique that provides, for the first time, constraints on the energy input flux at the coronal base ($r\sim\,1.025\,{\rm R}_\odot$) of the quiet-Sun at a global scale. By combining differential emission measure t
Externí odkaz:
http://arxiv.org/abs/1706.00365