On the Velocity and Intensity Asymmetries of Solar P-Mode Lines

Details On the Velocity and Intensity Asymmetries of Solar P-Mode Lines On the Velocity and Intensity Asymmetries of Solar P-Mode Lines

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ssrv...85..113g&link_type=abstract

Space Science Reviews, v. 85, Issue 1/2, p. 113-116 (1998).

Physics

Solar Oscillations

Scientific paper

We show that to explain the opposite line asymmetries shown by the
velocity and intensity spectra, it is necessary to solve the full
non-adiabatic problem which is at least of the fourth order.

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