Geology Reference
In-Depth Information
(a)
1.0
0.9
0.8
0.7
0.6
0.5
0.4
0.3
0.2
0.1
0.0
0
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
0.1
Cycles/kyr
(b)
JUL
AUG
SEP
150
100
OCT
50
NOV
DEC
JAN
FEB
0
−50
MAR
APR
MAY
JUN
−100
−150
0
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
0.1
Cycles/kyr
ETP/Mar
ETP/May
ETP/Jul
ETP/Sept
ETP/Nov
ETP/Jan
ETP/Apr
ETP/Jun
ETP/Aug
ETP/Oct
ETP/Dec
ETP/Feb
Figure 5.4 4π prolate multitapered coherency (a) and cross-phase (b) spectra of the ETP versus monthly insolation
at 35° North from 40 to 36 Ma, time increasing toward the present. ETP and monthly insolation were computed
using Analyseries 2.0.4.2 (Paillard et al. 1996); spectra were computed with cmtm.m by Peter Huybers (see Appendix).
High coherency and stable cross phase is detected in the eccentricity, obliquity, and precession index bands, as well as
in minor, high-frequency precession index bands at (14 kyr) −1 and (13 kyr) −1 . Source: Kodama, Anastasio, Newton,
Pares & L. A. Hinnov 2010. Reproduced with permission of John Wiley & Sons, Inc.
Figure 5.5 Timescales for the Arguis ARM cyclostratigraphy. 2π prolate multitaper power spectra on the left refer to
untuned and tuned ARM series on the right. (a) Original ARM series in the stratigraphic domain. (b) The ARM time
series according to GTS2004 magnetic reversal ages (GPTS2004). (c) The 405 kyr-tuned ARM time series, with 405 kyr tie
points indicated by vertical blue lines. The lowpass Taner filter isolates 405 kyr cyclicity. (d) La2004 eccentricity-tuned time
series, first iteration, shown with blue vertical lines between ARM minima and eccentricity minima. (e) La2004 eccentricity
tuning, second iteration. Minima and maxima of the lowpass filtered ARM series are tied to minima and maxima of the
eccentricity series, shown with blue vertical tie lines. (f ) La2004 precession index tuning of bandpassed precession band
of the eccentricity, second iteration tuned ARM series. (g) Depth-time transformation from each tuning. (h) ARM series
referring to the power spectra; the bottom-most series is the La2004 precession index-tuned accumulation rate series
defined at ~10 kyr intervals. The time picks were made using the “linage” function in Analyseries (Paillard et al. 1996);
see also picktune.m (Appendix).
 
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