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Hydromagnetic waves in Earth's core and their influence on ...

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209 Chapter 8 — Wave flowsIntegrat<str<strong>on</strong>g>in</str<strong>on</strong>g>g with respect to x∂B∂x − U η s<str<strong>on</strong>g>in</str<strong>on</strong>g> kx B = C 1. (8.56)The advecti<strong>on</strong>-diffusi<strong>on</strong> balance is therefore described by a 1st order ord<str<strong>on</strong>g>in</str<strong>on</strong>g>ary differentialequati<strong>on</strong>. The arbitrary c<strong>on</strong>stant C 1 will be zero if when x=0, dBdx = 0 also2 . If this isthe case then∂B∂x = U s<str<strong>on</strong>g>in</str<strong>on</strong>g> kx B. (8.57)ηSeparat<str<strong>on</strong>g>in</str<strong>on</strong>g>g the variables<str<strong>on</strong>g>and</str<strong>on</strong>g> then <str<strong>on</strong>g>in</str<strong>on</strong>g>tegrat<str<strong>on</strong>g>in</str<strong>on</strong>g>g∫ dBB = ∫ Uηs<str<strong>on</strong>g>in</str<strong>on</strong>g> kx dx, (8.58)ln B = − U kη cos kx + C 2, (8.59)so thatB(x, t) t→∞ = C 2 e − U kη cos kx . (8.60)To determ<str<strong>on</strong>g>in</str<strong>on</strong>g>e the amplitude of this steady state magnetic field, the c<strong>on</strong>stant C 2 must beevaluated <str<strong>on</strong>g>and</str<strong>on</strong>g> the <str<strong>on</strong>g>in</str<strong>on</strong>g>itial <str<strong>on</strong>g>and</str<strong>on</strong>g> steady state field strengths must be l<str<strong>on</strong>g>in</str<strong>on</strong>g>ked. This can beachieved follow<str<strong>on</strong>g>in</str<strong>on</strong>g>g the approach adopted by Clark (1965) <str<strong>on</strong>g>and</str<strong>on</strong>g> c<strong>on</strong>sider<str<strong>on</strong>g>in</str<strong>on</strong>g>g the <str<strong>on</strong>g>in</str<strong>on</strong>g>tegratedmagnetic field over <strong>on</strong>e wavelength of the wave flowddtπ∫k− π kB(x, t) dx. (8.61)S<str<strong>on</strong>g>in</str<strong>on</strong>g>ce the velocity field u is periodic <str<strong>on</strong>g>in</str<strong>on</strong>g> x (wavelength 2π k ), if the <str<strong>on</strong>g>in</str<strong>on</strong>g>itial field B 0 is uniform,then the steady state field B <str<strong>on</strong>g>and</str<strong>on</strong>g> its derivatives with respect to x(∂B∂x<str<strong>on</strong>g>and</str<strong>on</strong>g> ∂2 B∂x 2 )also always be periodic with the same period as u <str<strong>on</strong>g>and</str<strong>on</strong>g> will <str<strong>on</strong>g>in</str<strong>on</strong>g>tegrate to zero over the<str<strong>on</strong>g>in</str<strong>on</strong>g>terval ( −πk , π k). Therefore, return<str<strong>on</strong>g>in</str<strong>on</strong>g>g to the time dependent <str<strong>on</strong>g>in</str<strong>on</strong>g>ducti<strong>on</strong> equati<strong>on</strong>will∂B∂t+ U s<str<strong>on</strong>g>in</str<strong>on</strong>g> kx∂B∂x + Uk cos kxB = η ∂2 B∂x 2 , (8.62)<str<strong>on</strong>g>and</str<strong>on</strong>g> <str<strong>on</strong>g>in</str<strong>on</strong>g>tegrat<str<strong>on</strong>g>in</str<strong>on</strong>g>g from x = −πkto x = π k leavesddtπ∫k− π kB(x, t)dx = 0. (8.63)Physically this says that the amount vertical magnetic flux with<str<strong>on</strong>g>in</str<strong>on</strong>g> <strong>on</strong>e wavelength ofthe stati<strong>on</strong>ary wave pattern is c<strong>on</strong>served. This property then allows the flux with<str<strong>on</strong>g>in</str<strong>on</strong>g> a2 This cannot be rigorously established at this po<str<strong>on</strong>g>in</str<strong>on</strong>g>t. The analysis, however, proceeds <strong>on</strong> the assumpti<strong>on</strong>that C 1=0 <str<strong>on</strong>g>and</str<strong>on</strong>g> the assumpti<strong>on</strong> is justified a posteriori by the fact that the steady state soluti<strong>on</strong>found for B does <str<strong>on</strong>g>in</str<strong>on</strong>g>deed have this form.

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