Gr. Richards, ORBITAL FORCING AND ENDOGENOUS INTERACTIONS - NONLINEARITY, PERSISTENCE AND CONVERGENCE IN LATE PLEISTOCENE CLIMATE, Quaternary science reviews, 13(8), 1994, pp. 709-725
The succession of ice ages and interglacials during the late Pleistoce
ne has been linked with changes in the eccentricity, obliquity and pre
cession of the earth's orbit. The combined effect of orbital cycles wi
th different periodicities argues that climate should exhibit both per
sistence - significant dependence between observations at distant inte
rvals - and non-linearity. At the same time, a significant component o
f climatic variation derives from endogenous interactions which exhibi
t non-linear properties at both higher and lower frequencies than the
orbital variations. In order to analyze the effect of orbital shifts a
nd endogenous interactions, climate is factored into an orbitally forc
ed and a residual component. The component explained by orbital forcin
g shows some evidence of non-linearity, strong dependence between obse
rvations over the first 10 ka, and additional dependence between obser
vations at frequencies corresponding to the orbital cycles. The residu
al component shows greater dependence between observations over the fi
rst 20 ka, some evidence of dependence at the orbital cycles, and sign
ificantly greater degrees of non-linearity. Neither shows evidence of
actual chaoticity. The climatic residual generally moves in the same d
irection as the path implied by orbital forcing, meaning that endogeno
us interactions reinforce and accentuate changes in climate implied by
orbital shifts. Despite the high variability of the residual, orbital
forcing acts as a long-run attractor both for temperature and for atm
ospheric CO2. Actual temperatures converge to the path implied by orbi
tal forcing, on average within a period of 7.14 ka. Because orbital fo
rcing is a long-term attractor for temperature but short-term movement
s show strong serial dependence, the best forecasts for Pleistocene cl
imate are obtained from a model including distributed lags of both orb
ital shifts and temperature.