On the Balmer: Paschen ratio in prominences

Details On the Balmer: Paschen ratio in prominences On the Balmer: Paschen ratio in prominences

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...89...31p&link_type=abstract

Solar Physics, Volume 89, Issue 1, pp.31-33

Physics

Scientific paper

Vidicon data for the intensities of Balmer and Paschen lines for n = 11 to 18 indicate a line ratio within 1σ of the theoretical value of 3.27, calculated with the assumptions of an optically thin atmosphere and angular momentum substates populated according to their statistical weights. The observed value is not consistent with the value of 8 reported in some early work, or with the model that higher angular momentum states have low populations.

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