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Department of Earth and Planetary Sciences
Yale University
New Haven, CT
United States of America
I am a PhD candidate working with Professor Juan Lora in the Department of Earth and Planetary Sciences at Yale University. I investigate the dynamics of the middle atmosphere (stratosphere and mesosphere) of Saturn’s largest moon, Titan, using the Titan Atmospheric Model (TAM), a three-dimensional general circulation model. Much of what we know about Titan’s atmosphere was based on measurements of low-abudance molecules, which serve as atmospheric tracers. For example, observations of Titan’s middle atmosphere by the Voyager 2 and Cassini spacecraft, as well as recent high resolution observations from the ground-based Atacama Large sub-Mm Array, have measured an enrichment of trace molecules in the winter hemisphere. The winter polar enrichment is caused by a global summer-to-winter meridional overturning circulation that transports high altitude air towards the winter pole and delivers molecules from the high-altitude source regions to the winter stratosphere. Exactly how this circulation works has been the focus of my dissertation research.
General Circulation Models (GCMs) are computional models that solve the primitive equations of meteorology. Using GCMs allows us to simulate the complex states of planetary atmospehres 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 built on the GFDL FMS system. During my PhD, I added new modules to the model to capture the seasonally varying radiative heating due to the seasonaly in atmopsheric composition, as well as stabilize the upper-most levels of the model. These allowed us to better simulate the middle atmosphere of Titan, and resulted in multiple publications.
I've lead studies of Titan's atmosphere that used 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 datasets, I've made the first measurements of propene in the stratosphere, as well as the first detection of propadiene on Titan. By using different wavelengths of light, I've also made the deepest measurement of ethane in Titan's stratosphere, providing a useful constraint for photochemical and dynamical models.
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.