Energy relations on the small oscillations excitation in the stars

Details Energy relations on the small oscillations excitation in the stars Energy relations on the small oscillations excitation in the stars

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.220..195g&link_type=abstract

In ESA The Hydromagnetics of the Sun p 195-196 (SEE N85-25091 14-92)

Physics

Eddington Approximation, Stellar Oscillations, Work Functions, Energy Budgets, Heat Flux, Solar Flux

Scientific paper

It is shown that some derivations of the Eddington formula are
incorrect. However the formula of the work integral is correct because
it is the consequence of the linear equations of oscillations. The work
integral is equal to the change of the star oscillations energy over the
period but not total star energy.

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