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Upward and Downward Continuation of Potential Field on Spherical Patch Area using 2-Dim DFT

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2011 한국지구물리 ․ 물리탐사학회 학술대회 및 정기총회 2011년 10월 6일(목) ~ 7일(금), 한국지질자원연구원 강당동

구면상의 지역에서의 퍼텐셜마당에 대하여 2차원

푸리에변환을 이용한 위로 또는 아래로의 연속

나성호1), 정태웅2) 1)한국천문연구원 우주과학연구부, [email protected] 2)세종대학교 에너지자원공학과

Upward and Downward Continuation of Potential Field on

Spherical Patch Area using 2-Dim DFT

Sung-Ho Na1), Tae-Woong Chung2) 1)Space Science Research Center, KASI

2)Department of Energy and Resource Engineering, Sejong Univ

Two most important potential fields in geophysics are gravity field and stationary magnetic field. Sometimes we need to know the values of such field at a specified height, which is either higher or lower than original datum plane. Then downward or upward continuation of the field can be readily achieved by using two dimensional DFT (Discrete Fourier Transform), when the area is relatively small compared with the Earth's radius, In this study, we derive an algorithm for upward or downward continuation of gravity field on a spherical patch area. And this algorithm can be applied for any other potential field on spherical patch area. Gravity field vector  is expressed as the gradient of the gravity

potential , so that   ∇. Usually vertical component      

only is considered.

Laplace equation for a gravity potential field , like any other, in spherical coordinate is given as eq.(1).

∇        sin   sin   sin      (1)

Suppose we have a set of potential field data acquired on a spherical patch area, which has range of ≤  ≤  and ≤  ≤  with grid spacing of ∆ and ∆. We denote   ∆  ∆

as    and its Fourier transform as   . So their relations can be written as the following.

      

     

         exp     exp   (2a) 177

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나성호, 정태웅 2011 한국지구물리․물리탐사학회 학술대회 및 정기총회 178     

    

         exp     exp    (2b) Then the discrete version of Laplace eq. in terms of    is found as

    

             ∆        ∆     cot ∆  ∆      sin   ∆   exp  exp    

And it is claimed here that the coefficient of the summand vanishes, The resulting differential equation for    is written as        , (3a) with     ∆    ∆ cot ∆     ∆ sin  ∆  . (3b)

Eq.(3a) belongs to Euler-Cauchy differential eq. and its solution is given as    , where

    ±   ('-' should be taken here).

The continuation of gravity potential  can be done by the following procedure.    ⇒    ⇒    ⇒    

The three successive procedures are 1) Fourier transform, 2) 

        

 , and 3) inverse Fourier transform.

In practice, usually the gravity field itself is processed. The continuation of gravity field  is attained similarly.

   ⇒    ⇒    ⇒    

It should be noted that the exponent in the second procedure is replace by    due to the difference in radial dependence. Below are attached sample outputs.

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