These variations can be interpreted in terms of the paleoclimatic evolution of mid-latitude Chile and are compared to existing terrestrial records. Variations of rainfall in mid-latitude Chile are most likely controlled by shifts of the latitudinal position of the Southern Westerlies. Compared to the Holocene, the southern westerly wind belt was located significantly farther north during the last glacial maximum. 7.00 pm Peter Jost Enterprise Centre, JMU All are welcome and there is no charge for this meeting. Refreshments will be available from 6.30 pm.
Titan is one of the strangest places in the solar system.
Amateur astronomers can see Titan this week through a small telescope just after sunset. The CCNet is a scholarly electronic network. Information circulated on this network is for scholarly and educational use only. The attached information may not be copied or reproduced for any other purposes without prior permission of the copyright holders.