The empirical determination of line source functions, β L -values, and the microturbulent and convective velocity components as functions of depth in the photosphere-chromosphere transition region

Details The empirical determination of line source functions, β L -values, and the microturbulent and convective velocity components as functions of depth in the photosphere-chromosphere transition region The empirical determination of line source functions, β L -values, and the microturbulent and convective velocity components as functions of depth in the photosphere-chromosphere transition region

Aug 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972soph...25..277d&link_type=abstract

Solar Physics, Volume 25, Issue 2, pp.277-304

Physics

11

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1972SoPh...25..277D

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