CHIANTI
An Atomic Database for Spectroscopic Diagnostics of Astrophysical
Plasmas.
Naval
Research Laboratory (USA)
- Rutherford Appleton Laboratory
(UK)
University of Cambridge
(UK)
- George Mason University
(USA)
- Universita'
degli Studi di Firenze (Italy)
CHIANTI is an ongoing collaboration among researchers working
at the Naval Research Laboratory (USA), and
the Universities of Cambridge (UK), George Mason (USA), and
Florence (Italy).
Currently (2009), only CHIANTI team members in the USA
have some funds via an NRL (USA) grant.
We acknowledge having received in previous years some financial support from:
- Particle Physics and Astronomy Research Council (PPARC, UK)
- NASA - Ultraviolet, Visible and Gravitational Astrophysics grant (USA)
- NASA - Applied Information Systems Research Program grant (USA)
- NASA - Living With a Star grant (USA)
- NASA - Solar and Heliospheric Physics CHIANTI grant (USA)
- Chandra Emission Line Project (USA)
- NATO grant
- Agenzia Spaziale Italiana (ASI, Italy)
- Ministero dell'Istruzione dell'Universita' e della Ricerca (MIUR, Italy)
We are grateful to the individual scientists who made available to us the electronic files
of their calculations. These include:
- A.K. Bhatia (GSFC)
- M.F. Gu (Stanford)
- J. Dubau (Univ. Paris)
- J. Pelan, C.A. Ramsbottom, K. Bell (QUB)
- K.A. Berrington (Sheffield Univ.)
- C. Ballance (Rollins College)
- W.L. Wiese, W.C. Martin, A. Musgrove and T. Shirai (NIST)
- H.L. Zhang and A.K. Pradhan (OSU)
- D.H. Sampson (PSU)
- K.G. Widing (NRL)
- P.J. Storey (UCL)
- T. Kato (TU)
- U.I. Safronova (IS/RAS)
- S.S. Tayal (CAU)
Last revised by G. Del Zanna on 4-Sep-2009