A numerical method of adiabatic nonradial solar oscillation

Details A numerical method of adiabatic nonradial solar oscillation A numerical method of adiabatic nonradial solar oscillation

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996cha%26a..20..382b&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 20, Issue 3, p. 382-382.

Astronomy and Astrophysics

Astrophysics

Scientific paper

We adopt a modified parallel shooting method, that is, a continuous orthonormalization that avoids the difficulties of the original parallel shooting method, the proper choice for mesh size for different modes and the non-availability of a cost-effective way of improving the computed eigenfrequencies beyond a certain threshold. Using the modified method we calculated some low-order and low-degree solar p-mode and g-mode eigenfrequencies for the standard solar model and agreement with the observation at the 1% level was achieved.

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