Stanford Doerr School of Sustainability
Showing 1,251-1,260 of 1,428 Results
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Faye Shen Li Thijssen
Ph.D. Student in Environmental Social Sciences, admitted Autumn 2025
BioFaye is a PhD student in Environmental Social Sciences. Her research focuses on the political economy of the environment with a particular emphasis on how transnational corporations shape climate politics through their global political, social, and economic embeddedness. More specifically, she is currently investigating the extent to which the increasing material costs of climate vulnerabilities influence the power dynamics between pollutive industrial corporations (as employers) and the climate policy preferences of workers in these industries.
Prior to coming to Stanford, her research focused on indirect corporate influence in environmental politics, investigating executional greenwashing and its potential to affect public perceptions and preferences for regulatory policy. This research primarily employed experimental methods, with support from the Oxford Department of Politics & International Relations and the Nuffield Centre for Experimental Social Sciences. -
Leif Thomas
Professor of Earth System Science and, by courtesy, of Civil and Environmental Engineering and of Oceans
Current Research and Scholarly InterestsPhysical oceanography; theory and numerical modeling of the ocean circulation; dynamics of ocean fronts and vortices; upper ocean processes; air-sea interaction.
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Barton Thompson
Robert E. Paradise Professor of Natural Resources Law, Professor of Environmental Social Sciences and Senior Fellow at the Woods Institute for the Environment
BioA global expert on water and natural resources, Barton “Buzz” Thompson focuses on how to improve resource management through legal, institutional, and technological innovation. He was the founding Perry L. McCarty Director of the Stanford Woods Institute for the Environment, where he remains a Senior Fellow and directs the Water in the West program. He also has been a Senior Fellow (by courtesy) at Stanford’s Freeman-Spogli Institute for International Studies, and a visiting fellow at the Hoover Institution. He founded the law school’s Environmental and Natural Resources Program. He also is a faculty member in Stanford’s Emmett Interdisciplinary Program in Environment and Resources (E-IPER).
Professor Thompson served as Special Master for the United States Supreme Court in Montana v. Wyoming, an interstate water dispute involving the Yellowstone River system. He also is a former member of the Science Advisory Board of the United States Environmental Protection Agency. He chairs the boards of the Resources Legacy Fund and the Stanford Habitat Conservation Board, is a California trustee of The Nature Conservancy, and is a board member of the American Farmland Trust, the Sonoran Institute, and the Santa Lucia Conservancy.
Professor Thompson is of counsel to the law firm of O’Melveny & Myers, where he specializes in water resources and was a partner prior to joining Stanford Law School. He also serves as an advisor to a major impact investment fund. He was a law clerk to Chief Justice William H. Rehnquist ’52 (BA ’48, MA ’48) of the U.S. Supreme Court and Judge Joseph T. Sneed of the U.S. Court of Appeals for the Ninth Circuit. -
Sonia Tikoo-Schantz
Assistant Professor of Geophysics and, by courtesy, of Earth and Planetary Sciences
BioI utilize paleomagnetism and fundamental rock magnetism as tools to investigate problems in the planetary sciences. By studying the remanent magnetism recorded within rocks from differentiated planetary bodies, I can learn about core processes that facilitate the generation of dynamo magnetic fields within the Earth, Moon, and planetesimals. Determining the longevities and paleointensities of dynamo fields that initially magnetized rocks also provides insight into the long-term thermal evolution (i.e., effects of secular cooling) of planetary bodies. I also use paleomagnetism to understand impact cratering events, which are the most ubiquitous modifiers of planetary surfaces across the solar system. Impact events produce heat, shock, and sometimes hydrothermal systems that are all capable of resetting magnetization within impactites and target rocks via thermal, shock, and chemical processes. Therefore, I am able to use a combination of paleomagnetic and rock magnetic characterization to investigate shock pressures, temperatures, structural changes, and post-impact chemical alteration experienced by cratered planetary surfaces.
