Non-Gaussian Doppler profiles of spectral lines at the maxwellian velocity distribution

Details Non-Gaussian Doppler profiles of spectral lines at the maxwellian velocity distribution Non-Gaussian Doppler profiles of spectral lines at the maxwellian velocity distribution

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001kfnt...17..478k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 17, no. 5, p. 478-481

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Scientific paper

The case of the non-Gaussian Doppler profiles of spactral lines (at a small optical thickness of the investigation object) is considered. It is shown that such a sitiation may exist not only at the non-Maxwellian velocity distribution, but at the Maxwellian distribution as well. The reason is that turbulent elements may have different radiation intensities, which is a realistic assumption, but this was ignored in the analyses of solar flares and other astrophysical objects.

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