Geology Reference
In-Depth Information
so that
V≈ ρ( r 0 ) δ s
ρ d
δ r 0 dr 0 dS
= ρ( r 0 ) R
r 0 R 2 sinθ d θ d λ dr 0 ,
(5.148)
after substitution for δ s r 0 from (5.146). ρ( r 0 ) is to be interpreted as the density
on the equipotential with mean radius r 0 . Similarly, since the intensity of gravity is
inversely proportional to the orthometric separation of the equipotentials,
δ U i
= δ U i
δ r 0 δ r 0
g dS
δ s dS
δ s dS
1
(1/ R 2 ) (∂ R /∂θ ) 2
R /∂ r 0
+
dU i
dr 0
R 2 sinθ d θ d λ .
=
(5.149)
Together with the addition theorem (B.9),
n
1) k P n (cosθ) e ik λ P n (cosθ ) e ik λ
P n (cos
Θ
)
=
(
,
(5.150)
k =− n
(5.148) and (5.149) can be used to reduce (5.138), including (5.140), to the single
scheme
GP n (cosθ) d
r 0 ρ( r 0 ) π
R n 1 R
1
r 0 P n (cosθ )sinθ d θ dr 0
0
2 P n (cosθ) π
0
P n (cosθ )sinθ R
r 0
dr
( r ) n 1 d θ
+
2
Ω
dr 0 P n (cosθ) π
(1/ R 2 ) (∂ R /∂θ ) 2
R /∂ r 0
dU i
1
R n 1
1
+
P n (cosθ )sinθ d θ
+
0
2 GM
2 r 0 , n
2
3 Ω
=−
1,
2 U i
2 r 0 ,
n
=
0,
=
(5.151)
2 P 2 (cosθ), n
(2/3)
Ω
=
2,
0,
n
=
1,3,4,5, ··· .
In arriving at the relations (5.151), the following should be noted: all the terms in
the summation in the addition theorem for k 0 vanish on integration over azimuth;
and the second integral on the left of (5.138) over the volume
0 involves
integration over radius from r 0 to R , with R a function of θ , so the integration over
radius is to be completed before the integration over θ .
V
−V
i
Search WWH ::




Custom Search