Geoscience Reference
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we obtain the equation
D
d r ρ a d z
d
0 ρ w d z
d r
d
+
L
D
ρ w d z
+
=
+
ρ
( z )d z
+
L ρ a d z
(7.66)
0
d
d
+
Rearranging yields
L
( d d r )( ρ a ρ w ) =
( ρ ( z ) ρ a )d z
(7.67)
0
To determine
ρ
( z ), we must use the expression for density as a function of
temperature and
α
the coefficient of thermal expansion,
ρ ( T ) = ρ a [1 α ( T T a )]
(7.68)
and Eq. (7.61) for the temperature structure of the lithosphere. Substituting these
two equations into Eq. (7.67)gives
( d d r )( ρ a ρ w ) = ρ a α T a
erfc
d z
L
z
2 κ t
(7.69)
0
where erfc is the complementary error function (see Appendix 5). The integral
on the right-hand side of this equation can easily be calculated or looked up in
a set of mathematical tables. However, for our purposes it is sufficient to change
the upper limit of integration from L to
(the error introduced by this approx i-
mation is about 5%). This integral of erfc( x ) between x
/ π
=
0 and infinity is 1
(Appendix 5). When this approximation is made, Eq . (7 .69) becomes
T a κ t
π
( d
d r )(
ρ a ρ w )
=
2
ρ a α
(7.70)
Rearranging Eq. (7.70)gives
κ t
π
2 ρ a α T a
ρ a ρ w
d = d r +
(7.71)
10 3
10 3 kg m 3 ,
If we assume values for
ρ a and for
ρ w of 3.3
×
and 1.0
×
,10 6 m 2 s 1 ; for T a , 1200 C; and for
d r , 2.6 km; with t in millions of years and d in kilometres, then Eq. (7.71)is
d
10 5 C 1 ; for
respectively; for
α
,3
×
κ
33 t
=
2
.
6
+
0
.
(7.72)
When T a is taken to be 1300 C, Eq. (7.71)is
d = 2 . 6 + 0 . 36 t
(7.73)
Such dependence of ocean depth on age is in broad agreement with the depths
observed for oceanic plates less than 70 Ma old (Eq. (7.57a)). Thus, as the litho-
sphere moves away from the ridge axis, it cools, contracts and hence subsides.
Table 7.4 gives the details of the physical parameters for oceanic-lithosphere
thermal models.
The boundary-layer or half-space models
The boundary-layer model is a modification of the simple half-space model:
the rigid lithosphere is assumed to be cooled asthenosphere, and the base
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