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Published byBaldric Maximillian Shields Modified over 6 years ago
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(W is scalar for displacement, T is scalar for traction)
Note that matrix does not depend on m
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Algorithm for toroidal modes
Choose harmonic degree and frequency Compute starting solution for (W,T) Integrate equations to top of solid region Is T(surface)=0? No: go change frequency and start again. Yes: we have a mode solution
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T(surface) for harmonic degree 1
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Radial and Spheroidal modes
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Spheroidal modes
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Minors To simplify matters, we will consider the spheroidal mode equations in the Cowling approximation where we include all buoyancy terms but ignore perturbations to the gravitational potential
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Spheroidal modes w/ self grav
(three times slower than for Cowling approx)
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Red > 1%; green .1--1%; blue .01--.1%
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Red>5; green 1--5; blue .1--1 microHz
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Mode energy densities
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Normalized radius Dash=shear, solid=compressional energy density
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(black dots are observed modes)
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All modes for l=1
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(normal normal modes)
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hard to compute ScS --not observed (not-so-normal normal modes)
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