Analysis of Balmer /α intensity measurements near solar minimum

Details Analysis of Balmer /α intensity measurements near solar minimum Analysis of Balmer /α intensity measurements near solar minimum

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001jastp..63..341b&link_type=abstract

Journal of Atmospheric and Solar-Terrestrial Physics, Volume 63, Issue 4, p. 341-353.

Physics

11

Scientific paper

Balmer /α intensity measurements made with a dual etalon Fabry-Perot spectrometer at Haleakala during two campaigns in 1988 are presented. The data from each campaign demonstrate night-to-night stability, despite variations in geophysical conditions. Analysis of these data using a nonisothermal Lyman /β radiative transport code, updated solar Lyman /β line-center flux estimates, and corrected thermospheric atomic hydrogen density profiles points to the resolution of the ``factor of 2'' problem. A careful reassessment of other mechanisms for upper atmospheric Balmer /α excitation has also been carried out.

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