The Atmosphere; Its Characteristics And Dynamics

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+ ^ log cos t? + ^, (12) where the capitals are constants in general.
In order to determine the constants in Equation (12) it would be necessary to observe the polar velocities at six points, although theoretically Equation (10) would only require three points. These equations are utterly unmanageable in practice.
However, they may be reduced by the aid of series. Since a function ■can be expressed as a series by the aid of Maclaurin's theorem, which is / ('^) =/ (o) + */'(^) + ^ Ao) + ~ f'lo)
...etc., we can develop the functions in Equation (12) into the following forms, by neglecting powers of '* above the third.
2 .51° cos 2 '? = I — 2 »\ tan .? = .!>-] -.
3 ■ 03 . Q a tan" t!> = — 7-- log cos '? = .
3 ! "^ 2 Substituting these expressions in Equation (12) we have, V=-^(l-2^") + ^(^ + l^)-C(?^)-i?*-£^+^. (13) Reducing and again letting capitals express constants in general (not the same as before), we have v;^A^-B&^-{-C> are, of course, expressed here in radians.


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