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Comments on the Measurement of Transition Probabilities

Published online by Cambridge University Press:  25 April 2016

Martin C E Huber  and
Ursula Pauls
Martin C E Huber
Affiliation:
Swiss Federal Institute of Technology Zurich (ETHZ), Institute of Astronomy and Physical Chemistry Laboratory, ETH-Zentrum, CH-8092 Zurich, Switzerland
Ursula Pauls
Affiliation:
Swiss Federal Institute of Technology Zurich (ETHZ), Institute of Astronomy and Physical Chemistry Laboratory, ETH-Zentrum, CH-8092 Zurich, Switzerland

Extract

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Developments in the measurements of oscillator strengths, that are of current and future interest to astrophysics, have taken place in the past few years:

  1. – there is increased emphasis on methods which are independent of level populations (i.e., of number densities and thus equilibrium in the vapour or plasma under investigation),

  2. – clear progress has been made towards higher precision (and accuracy) and

  3. – the dynamic range of astrophysically relevant oscillator strengths was further extended towards weaker lines.

Type
Chapter IV Reports of Meetings of Commissions
Information
Transactions of the International Astronomical Union , Volume 19 , Issue 2 , 1985 , pp. 153 - 155
Copyright
Copyright © Reidel 1985

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