Atlas of Deep-Water Outcrops

Tor H. Nilsen, a red-haired Scandinavian who stood more than six feet tall, died October 9, 2005, at his San Carlos, California, home. This was after a valiant five-year fight with melanoma cancer. He was 63. His ashes were scattered at his family plot in Norway in 2006.
He was born in New York City on November 29, 1941, to Mollie Abrahamson and Nils Marius Nilsen of Mandal, Norway, and was the first of their children to be born in the United States. After graduating from Brooklyn Tech, he earned his B.S. in geology from City College of New York in 1962. While there, his prowess on the basketball court impressed a scout from the New York Knicks, but Tor went on to graduate school and earned his M.S. and Ph.D. degrees in geology from the University of Wisconsin at Madison in 1964 and 1967, respectively. His M.S. thesis was a study of Precambrian metasedimentary deposits in the Lake Superior area, and his Ph.D. thesis was a study of Devonian alluvial-fan deposits of the Old Red Sandstone in western Norway.
Dr. Nilsen’s principal expertise was in depositional systems analysis, stratigraphic analysis, and the relationships among tectonics, eustasy, and sedimentation. He began his industry career in 1967 as a research geologist with the Shell Development Company in Houston, Texas, and Ventura, California, where he worked on the tectonics and sedimentation of Tertiary shelf systems of coastal California. He subsequently spent two years with the U.S. Army Corps of Engineers as the Military
A Prograding Miocene Turbidite System, Tempa Rossa Cliffs, Italy
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Published:January 01, 2008
Abstract
Along the coast of southern Italy, near Tempa Rossa, is an outcrop with a turbidite succession greater than 150 m (460 ft) thick. It is part of the Pollica Sandstones Formation, which is the oldest formation of the Cilento Group (Miocene [Langhian to Lower Tortonian]). The Cilento Group (Pollica and the overlying San Mauro Formation) was deposited in a wedge-shaped basin above deposits that were formed during the early phases of the formation of the Southern Apennines. The Pollica Formation is comprised of several channelized deposits of coarse- and very coarse-grained siliciclastic units. These are capped by and laterally grade into fine-grained facies and chaotic deposits. The S. Mauro Formation, thicker than the Pollica, is composed of fine-grained carbonates (re-sedimented pelagic and hemipelagic biogenic oozes) that occur in discrete beds (up to 60 m [190 ft] thick), alternating with fine- to medium-grained, laterally continuous, siliciclastic units.