Find my email at the Department website below
Department of Earth and Planetary Sciences
Yale University
New Haven, CT
United States of America
I am a PhD candidate in Planetary Climate Dynamics working with Professor Juan Lora in the Department of Earth and Planetary Sciences at Yale University. My research expertise is in the field of geophysical fluid dynamics, which is the study of how liquids and gases move on planetary scales. Geophysical fluid dyanmics is used to explain phenomena like why the prevailing winds in the continental United States are from the west while they're from the east above the equator, why the California ocean current is cold and the Gulf Stream is warm, and why the temperature in the tropical Pacific impacts snowfall in Connecticut.
My primary research investigates the dynamics of the middle atmosphere (stratosphere and mesosphere) of Saturn’s largest moon, Titan. Like Earth, Titan has an atmosphere composed mostly of molecular nitrogen, though unlike Earth the second most abundant molecule is methane. The chemistry that results from the interactions between these two molecules leads to a complex world with diverse surface geomorphological features like dunes, riverbeds, and lakes, as well as a range of weather patterns that mirror attributes of Earth's own weather. I use a range of tools, from new observations from the world's leading telescopes and space observatories to state-of-the-art computational circulation models to determine the underlying physical mechanisms that govern this enigmatic world. Read more about my research interests on Titan below.
My background also extends into Earth-based oceanography through the study of wave propagation in the Arctic ocean through the analysis of data from the Beaufort Gyre Exploration Project. Read more about that here!
General circulation models (GCMs) are computational tools that solve the primitive equations of meteorology. Using GCMs allows us to simulate the complex states of planetary atmospheres and oceans, providing access to immense datasets of simulated variables, including winds, temperatures, and compositions. I work with the Titan Atmospheric Model (TAM) which was developed by my advisor, Professor Juan Lora, and is built on the GFDL FMS system. During my PhD, I developed new features to the model to capture the impact of Titan's seasonally varying composition on its circulation structure, as well as explore how the circulation drives the seasonally varying composition.
I've lead studies of Titan's atmosphere with data from the Composite Infrared Spectrometer (CIRS) on the Cassini spacecraft and the Texes Echelon Cross Echelle Spectrograph (TEXES) on the NASA Infrared Telescope Facility (IRTF) on Mauna Kea. With these data, I've made the first measurements of propene in the stratosphere, as well as the first detection of propadiene on Titan. Through different wavelengths of light, I've also made the deepest measurement of ethane and hydrogen isocyanide in Titan's stratosphere, which provide critical constraints for photochemical models to better simulate the chemistry that occurs in Titan's organic-rich atmosphere.
Fall 2024 PHYS 126 University Physics II
Spring 2024 PHYS 126 University Physics II Lab
Spring 2023 PHYS 122 General Physics II Lab
Fall 2023 EPS 274 Fossil Fuels and World Energy
Fall 2019 G&G 140 Introduction to Atmosphere, Ocean, and Climate Change
Collaborator on this project.