Information on transition probabilities of rare gas spectra is essential if radiative processes which occur in atomic discharges are to be fully understood. This need encompasses a range of disciplines, including astrophysics, plasma physics, and laser physics. It is often difficult in practice, however, to use published tables to their fullest extent by manual inspection and calculation because of the sheer bulk of data contained therein.
You do not have subscription access to this journal. Cited by links are available to subscribers only. You may subscribe either as an OSA member, or as an authorized user of your institution.
Contact your librarian or system administrator
Login to access OSA Member Subscription