Asymptotic structure in torsional free oscillation data for the Earth

Details Asymptotic structure in torsional free oscillation data for the Earth Asymptotic structure in torsional free oscillation data for the Earth

Aug 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974natur.250..400a&link_type=abstract

Nature, Volume 250, Issue 5465, pp. 400-401 (1974).

Physics

4

Scientific paper

THE eigenfrequencies, nσl of the torsional modes, n T l, of a spherically symmetrical, nonrotating, elastic, isotropic Earth model, are defined, for fixed wave number k=(l+ 1 2 )/a, by the eigenvalue problem (where U=U(r); μ = μ(r) ρ = ρ(r) a <= r <= b) and by the (zero stress) boundary conditions where μ, denotes rigidity, ρ density, a the radius of the core and b the radius of the Earth1.

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