On the possibility of investigating the solar wind using the Raman scattering spectral line 6825Å

Details On the possibility of investigating the solar wind using the Raman scattering spectral line 6825Å On the possibility of investigating the solar wind using the Raman scattering spectral line 6825Å

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471..301k&link_type=abstract

The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 301-304 (1999).

Computer Science

Particle Emission, Solar Wind, Visible

Scientific paper

The emission line λ6825Å that is due to Raman scattering of the radiation of OVI λ1032Å ions on the neutral hydrogen atoms has been found in solar spectrum. This line has the absorption component shifted to the short-wave range in the spectrum. The value of the Doppler shift corresponds to the line-of-sight velocities of the motion of the Sun's matter in the range of heights of the spectral line formation of about 300 km/s that agrees well with SOHO results.

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