Postdoc @ Stanford (Hansen Experimental Physics Lab). I build signal processing and statistical pipelines for weak signal detection in noisy, high-dimensional data, currently applied to the solar interior and atmosphere via helioseismology. Python, spectral analysis, FFTs, time series, uncertainty quantification, observational and numerical modeling. PhD in Astronomy (NMSU).
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Focusing
Postdoc at Stanford University
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Eclipse-AGW-Analysis
Eclipse-AGW-Analysis PublicAnalysis pipeline for detecting and characterizing atmospheric gravity waves (AGWs) from radiosonde data collected during solar eclipses using wavelet analysis and Stokes parameters.
Python
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Grey-Stellar-Atmosphere-Model
Grey-Stellar-Atmosphere-Model PublicGray LTE stellar atmosphere model for an A0V star using OPAL opacities, Saha ionization, and the Schwarzschild convection criterion.
Python 1
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magneto-rossby-dashboard
magneto-rossby-dashboard PublicInteractive Streamlit dashboard for visualizing magneto-Rossby and Alfvén wave dispersion relations on a sphere as a function of azimuthal order and magnetic field strength.
Python
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