Geoscience Reference
In-Depth Information
with a total lack of inconsistent dates, does the use of consistent dates yield
signi￿cantly better results. The log-likelihood function is beehive-shaped. This
topic will be discussed in more detail in the next sections.
3.1.1 Weighting Function Defined for Inconsistent Dates
Only Model
Cox and Dalrymple ( 1967 ) developed their statistical approach for estimating the
age of boundaries between polarity chronozones in the Cenozoic (Brunhes,
Matuayana, Gauss and Gilbert chronozones). A slightly modi￿ed version of their
method was used in Harland et al. ( 1982 ) for estimating the ages of boundaries
between the stages of the Phanerozoic geologic timescale as follows. Suppose that
t e represents an assumed trial or “estimator” age for the boundary between two
stages. Then the n measured ages t in the vicinity of this boundary can be classi￿ed
as t y (younger) or t o (older than the assumed stage boundary). Each age determina-
tion t yi or t oi has its own standard deviation s i . If these standard deviations are
relatively large, a number ( n a ) of the age determinations is inconsistent with respect
to the estimator t e. Only the n a inconsistent ages t ai with t oi <
t e were
used for estimation by Cox and Dalrymple ( 1967 ) and Harland et al. ( 1982 ). These
inconsistent ages may be indicated by letting i go from 1 to n a . In Harland
et al. ( 1982 ) the quantity E 2 with
t e and t yi >
X n a
i ¼1
2
E 2
s t
¼
ð
t ai
t e
Þ
=
is plotted against t e in the chronogram for a speci￿c stage boundary. Such a plot
usually has a parabolic form, and the value of t e for which E 2 is a minimum can be
used as the estimated age of the stage boundary.
The preceding approach also can be formulated as follows: Suppose that a stage
with upper stage boundary t 1 and lower boundary t 2 is sampled at random. This
yields a population of ages t 1 <
t 2 with uniform frequency density function h ( t ).
Suppose further that every age determination is subject to an error that is normally
distributed with unit variance. In general, the frequency density function f ( t )of
measurements with errors that satisfy the density function
t
<
ˆ
for standard normal
distribution satis￿es:
Z 1
1 ˆ
Z t 2
t 1 ˆ
1
t 2 t 1
1
t 2 t 1 ʦ
f t
ðÞ ¼
ð
t
x
Þ
ht
ðÞ
dx ¼
ð
t
x
Þ
dx ¼
ð
t
t 1
Þ
ʦ
ð
t
t 1
Þ
½
½
For this derivation, the unit of t can be set equal to the standard deviation of the
errors. Alternatively, the duration of the stage can be kept constant whereas the
standard deviation (
˃
) of the measurements is changed. Suppose that t 2
t 1 ¼
1, then
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