Issue |
Astron. Astrophys. Suppl. Ser.
Volume 136, Number 2, April II 1999
|
|
---|---|---|
Page(s) | 385 - 394 | |
DOI | https://doi.org/10.1051/aas:1999466 | |
Published online | 15 April 1999 |
Atomic data from the IRON Project
XXXIV. Electron impact excitation of Fe xvi
1
Lehrstuhl für Theoretische Physik I, Ruhr-Universität, D-44780 Bochum, Germany
2
Departamento de Física, Universidad Metropolitana, PO Box 76819, Caracas 1070A, Venezuela
3
UMR 8631 (associée au CNRS et à l'Université Paris 7) et DAEC, Observatoire de Paris, F-92195 Meudon, France
4
Centro de Física, Instituto Venezolano de Investigaciones Científicas (IVIC), PO Box 21827, Caracas 1020A, Venezuela
Send offprint request to: C.J. Zeippen
Received:
25
September
1998
Accepted:
18
November
1998
As part of the IRON Project, electron impact excitation effective collision strengths are computed for the ion Fe xvi familiar in solar spectra. A Breit–Pauli R-matrix calculation is performed with a 12-level () target representation. The calculation for this relatively simple ion is approached as a test case where we can analyze in detail most of the effects that contribute to the accuracy of the collision strengths: the energy mesh, relativistic corrections, the asymptotic multipole potentials and contributions from high partial waves. By comparing with two recent independent calculations, an accuracy rating of 10% is assigned to the present effective collision strengths in the electron-temperature range of .
Key words: atomic and molecular data / sun: corona
© European Southern Observatory (ESO), 1999