Spectral line and white-light intensities in the corona in the presence of propagating or standing shocks

Details Spectral line and white-light intensities in the corona in the presence of propagating or standing shocks Spectral line and white-light intensities in the corona in the presence of propagating or standing shocks

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..129..153e&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 129, Sept. 1990, p. 153-163.

Physics

4

Line Spectra, Luminous Intensity, Shock Wave Propagation, Solar Corona, Standing Waves, Interplanetary Space, Lyman Alpha Radiation, Shock Fronts, Solar Wind

Scientific paper

The effect of a propagating shock on the H I Ly-alpha line and the polarization brightness in the inner solar wind region is investigated. The shock produces measurable changes in both, and, provided the measurements are made simultaneously, the alteration of the density and velocity across the shock can be derived. For a standing shock, the effect of the Ly-alpha line and the white-light radiation is much smaller.

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