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6.18 Periodic heating of the surface          175

            The skin depth for daily variations of the surface temperature is 0.17 m and for yearly
            variations 3.2m.
              The temperature with units follows directly from the dimensionless solution. We just
                                ˆ
            insert the definitions for T , ˆz and ˆ t in equation (6.272) and get
                                               ω               ω

                           T (z, t) =  T exp −   z cos ωt −      z .          (6.273)
                                               2κ              2κ
            The solution in this form shows that variations with high frequencies die out with depth
            much faster than variations with low frequencies. Depth therefore acts as a filter that
            removes high-frequency variations in the surface temperature.
              We have already seen that we can add temperature solutions to obtain a new solution,
            because the temperature equation is linear. We can for instance add the stationary solution
            az + b, given by a constant thermal gradient a and constant average surface temperature
            b. Another possibility is to add together the solutions with different amplitude  T i and
            frequency ω i ,

                                                ω i              ω i

                         T (z, t) =   T i exp −    z cos ω i t −   z .        (6.274)
                                                2κ               2κ
                                   i
            This solution solves the problem with periodic surface temperature variations of the form

                                      f (t) =   T i cos(ω i t)                (6.275)
                                             i
            and such a general Fourier series can be used to approximate almost any kind of periodic
            surface temperature.
              Figure 6.36 shows observations of the temperature at the depths 1.2 m, 4 m and 9 m
            over a time span of 2 years and 4 months (Isaksen and Sollid, 2002). The data set is from a
            site with permafrost on the island of Svaldbard. We notice that there are weekly variations
            in the temperature data at 1.2 m depth, and that these high frequency variations have died
            out at 4 m where the temperature signal is smooth. We have that l 0 ≤ 0.6 m for variations
            with a period up to 1 month, and these variations are reduced to nearly zero (by a factor
                                                                               2 −1
            1/100) at the depth 6l 0 = 3.9 m. The model (6.273) is plotted for κ = 1 · 10 −6  m s  ,
                                              ◦
             T = 9.2 C, and a constant offset −6.3 C has been added. The model does not match
                     ◦
            the data at 4 m and 9 m, although weekly variations are filtered away, because there are
            variations in the observations with a period longer than a year.
            Note 6.10 The temperature equation (6.270) with boundary conditions (6.271)issolved
            by the separation of variables, T (ˆz, ˆ t) = U(ˆ t)V (ˆz). When the product U(ˆ t)V (ˆz) is inserted
                                    ˆ
            into the temperature equation (6.270) we get
                                        U     V
                                          =     = a + ib.                     (6.276)
                                        U    V

            These two ratios have to be equal to a constant (a+ib), because U /U is only a function of

            ˆ t and V /V is only a function of ˆz. The constant is the complex number a+ib where a and
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