Deep-water (below wave base) processes, although generally
hidden from view, shape the sedimentary record of more than 65% of
the Earth’s surface, including large parts of ancient
mountain belts. This book aims to inform advanced-level
undergraduate and postgraduate students, and professional Earth
scientists with interests in physical oceanography and hydrocarbon
exploration and production, about many of the important physical
aspects of deep-water (mainly deep-marine) systems.
The program will prepare the future leaders in the management of the natural resources value chain across the globe. The successful graduate from this program will be well versed in all aspects of the energy and natural resources industries, will be an effective communicator, will have a strong background in Earth Science and Engineering, will be aware of social responsibilities, will operate within international constraints and opportunities, and will have strong managerial skills. More...
Rock & Ice Physics Laboratory
Shackleton Ice Shelf is an extensive ice shelf fronting the coast of East Antarctica for about 384 km (95E to 105E), projecting seaward about 145 km in the western portion and 64 km in the east
The Rock Physics Laboratory
Mount St. Helens is an active stratovolcano located in Skamania County, Washington, in the Pacific Northwest region of the United States.
Experimental & theoretical rock physics, ice mechanics & petrologyapplied to planetary dynamics, geohazards, sub-surface reservoirs & ice sheets
The Rock & Ice Physics Laboratory (RIPL) at UCL is a major research facility which forms part of the Earth Sciences Department. RIPL has over 15 members and consists of 11 laboratories, housing over £4M of research equipment., supported by over £2 million of current peer-reviewed funding. The Rock & Ice Physics Laboratory has a unique breadth of experience and ability to design and build its own experimental apparatus.
We study the physical behaviour of ice and rocks that make up the surface and interior of the Earth, and other solid bodies in the solar system, so as to constrain the dynamic, tectonic and environmental processes of planetary evolution. Our research is nationally unique and multi-disciplinary, being based on experiment and theory.