fig03.htm

Figure 3. Time changes (thousand years) of (a) eccentricity, (b) tilt of the Earth's axis (in degrees), and (c) climate precession, ecdot( sin w) , multiplied by ( -1 ), where w is the longitude of the perihelion relative to the Spring Equinox point (after [{\it Berger and Loutre,} 1991]).


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