Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...254..436b&link_type=abstract
Astronomy and Astrophysics, Vol.254, NO. FEB(I), P. 436, 1992
Astronomy and Astrophysics
Astrophysics
128
Excitation Rate Coefficient, Positive Ions Spectroscopy, Corona, Data Compaction
Scientific paper
This paper presents a new way of critically assessing and compacting data for electron impact excitation of positive ions. Collision strengths Ω are scaled and then plotted as functions of the colliding electron energy, the complete range of energies being mapped onto the interval (0, 1). The scaled Ω can then be represented to good accuracy by a 5-point spline. Similar scaling and spline fitting techniques enable thermally averaged collision strengths Y to be obtained at all temperatures. Whole isoelectronic sequences may then be treated by mapping the ion charge onto (0, 1) and using a second 5-point spline; thus reducing Y, for the whole sequence and all temperatures, to a 5 × 5 array. Three main types of transition (optically allowed, forbidden and exchange) are discussed separately and illustrated by numerical examples. Interactive programs for analysing atomic data in this way have been developed.
Burgess Andrew
Tully John A.
No associations
LandOfFree
On the Analysis of Collision Strengths and Rate Coefficients does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with On the Analysis of Collision Strengths and Rate Coefficients, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the Analysis of Collision Strengths and Rate Coefficients will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1044758