Jökull


Jökull - 01.12.1973, Side 44

Jökull - 01.12.1973, Side 44
purpose. We can select a matrix B with a stronger negating power than A'. This would reduce equations (10) to an underdetermined problem BAx0 = Bb (33) which would then have to be treated by the methods described above. As will be discussed below there are cases where such an overnega- tion is convenient. The adjoint A' is optimal in the sense that it negates those and only those components of b which have to be negat- ed for the inversion of A. AN EXAMPLE FROM POTENTIAL THEORY In the following we will discuss an example from potential theory which is of interest in the interpretation of marine magnetic field anomalies. These anomalis are believed to re- sult from the magnetization of thin layers of lava at the ocean floor (Carmichael, 1970). Consider a horizontal magnetic stratum X carrying a unidirectional vertically oriented magnetization of density u(S) where S are the points on X- We will place the (x, y) plane in X with the z-axis vertical. Moreover, for the purpose of simplification let u(S) depend on the x-coordinate only and let u = 0 for x out- side the interval (0, L). We have then a one- dimensional case where u(x) has a bounded support. Using MKS units we find (Grant and West, 1965) that the scalar magnetic potential v(x, z) due to X a field point (x, z) is v(x, z) - (z/2tr) j u(x')dx' Z2+ (x-x')2 (34) The vertical magnetic field is K (x, z) = - fi0 (3v/3z) (35) which can also be expressed v(x,z) = - J bz(x, z')dz' (36) AC z Assuming that the magnetic field can be ob- served in a horizontal plane located at a dist- ance h above X> the fundamental problem of magnetic field interpretation consists in deriv- ing u(x) on the basis of the observed bz(x, h). This is equivalent to solving the integral equa- tion (34) for u(x) when z = h and v(x, h) is obtained on the basis of (36). The latter step is a simple integration obtained on the basis of an outward continuation of bz(x, h) which presents no formal difficulties. Equation (34) is an integral equation of the first kind where the operation on the right is a simple convolution. Hence, the most con- venient method of solution consists in applying the Fourier transformation with respect to x to (34). Let U(k) and V(k, h) be the transforms of u(x) and v(x, h), respectively, where k is the transform variable, that is, the wave-number in the transformed space. Using ■ transform tables (.Duff and Naylor, 1966) we find that the trans- formed version of (34) is V(k,h) = (i/2)exP(-|h|k)U(k) (37) and hence U(k) = 2 exp(|h|k)V(k, h) (38) which formally represents the Fourier trans- form of the solution of (34). Unfortunately, the exponential factor on the right of (38) is unbounded as k-^=° and does not possess an inverse transform. We are therefore unable to retrieve u(x) from U(k) unless re- strictions are imposed on V(k,h) so that the product on the right of (38) can be inverted. The integral equation (34) for u(x) is simply an improperly posed mathematical problem. This is evidenced by the fact that as k-»<® the ex- ponential factor in (38) causes an unbounded magnification of the high-frequency compon- ents of v(x, h). This situation is typical for many problems in interpretation theory. Equa- tion (34) is one of the most elementary ex- amples of an improperly posed interpretation problem. The simplest and most obvious way out of this difficulty is to reject any high-frequency components of v(x, h) beyond a certain cutoff wavenumber k0. Adopting this procedure, we 42 JÖKULL 23. ÁR
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