Geoscience Reference
In-Depth Information
Fig. 3.3 Caerfai St. David's boundary example. Age estimated by maximum likelihood method
using
L
. Standard deviation (
s
) and width of 95 % condence interval are approximated closely by
results shown in Fig.
3.2
(Source: Agterberg
1990
, Fig. 3.14)
E
2
points upwards in order to facilitate comparison with
chronograms in Harland et al. (
1982
).
Figure
3.3
shows estimates based on
L
. The resulting best-tting parabola is
almost equal to the one in Fig.
3.2
that was based on
L
a
instead of
L
. Consequently,
the estimated ages of the Caerfai-St David's boundary and their standard deviations
obtained from
L
a
and
L
also are similar. This conclusion will be corroborated by a
more detailed comparison of the weighting functions for
L
and
L
a
at the end of this
section, and by computer simulation experiments to be described in the next
section. However, it will be shown that
L
a
does not provide a good approximation
when inconsistent data are missing. When
n
is small,
L
also produces better results
than
L
a
because a parabolic chronogram is more readily obtained when the consis-
tent ages are used together with the inconsistent ages as will be illustrated by the
following example. An age estimate based on Harland et al.'s (
1982
, Fig. 3.4h,
p. 54) chronogram for the Norian-Rhaetian boundary is 213 Ma. The corresponding
standard error reported by Harland et al. (
1982
) is 9 Ma. The
L
-based maximum
likelihood method using the same data set of only six dates gives an estimated age
of 215.5 Ma with standard error of 4.2 Ma.
been inverted so that -
y
¼
3.1.4 The Chronogram Interpreted as an Inverted
Log-Likelihood Function
The approach taken in this section differs slightly from the one originally taken by
Cox and Dalrymple (
1967
). The basic assumptions that the dates are uniformly
distributed through time and subject to measurement errors are made in both
Search WWH ::
Custom Search