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CHIANTI An Atomic Database for Spectroscopic Diagnostics of Astrophysical Plasmas USER GUIDE – 11 Mar 2014 Written by Giulio Del Zanna with contributions from P.Young, E.Landi, K.Dere, H.Mason
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Document Date: 2014-03-13 12:03:09


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City

Cambridge / Washington / Florence / /

Company

Spectroscopic Diagnostics / Naval Research Laboratory / Rutherford Appleton Laboratory / Mn Co / /

Country

United States / Italy / United Kingdom / /

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Facility

Rutherford Appleton Laboratory / George Mason University / University of Florence / University of Michigan / University of Central Lancashire / Naval Research Laboratory / University of Cambridge / Arcetri Astrophysical Observatory / /

IndustryTerm

energy levels / high-energy configurations / observed energy levels / structure energy levels / observed energy / lower energy level / satellite lines / software changes / Energy difference / theoretical energy / upper energy level / energy / /

Organization

Department of Applied Mathematics and Theoretical Physics / University of Cambridge / University of Florence / George Mason University / University of Central Lancashire / the University of Michigan / /

Person

Peter Young / Ken Dere / Barbara Bromage / Brunella MonsignoriFossi / Gordon Bromage / Monsignori Fossi / H.Mason Contents / Dave Pike / Giulio Del Zanna / Enrico Landi / Massimo Landini / Helen Mason / /

Position

representative / /

ProgrammingLanguage

Python / /

ProvinceOrState

Michigan / /

Technology

radiation / X-ray / ascii / recombination / /

URL

http /

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