Submillimeter hydrogen lines in solar prominences

Details Submillimeter hydrogen lines in solar prominences Submillimeter hydrogen lines in solar prominences

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pazh....5...47b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 5, Jan. 1979, p. 47-49.) Soviet Astronomy Letters, vol. 5, Jan.-Feb. 1979, p. 27, 28. T

Physics

1

H Lines, Solar Prominences, Submillimeter Waves, Optical Thickness, Quantum Numbers, Solar Physics, Solar Spectra, Solar Temperature

Scientific paper

The parameters of hydrogen-line transitions of the type (n + 1) to n occurring in solar prominences are considered for principal quantum numbers in the range 10-25. Observations of these lines, which will appear at submillimeter wavelengths (40-1000 microns), not only afford an independent method for determining the density and temperature in prominences, but they would also provide a test of the theory of recombination-line broadening. Under favorable conditions the brightness temperature of the lines could reach 1000 K.

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