3D coronal mass ejection flux rope modeling
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Updated
Apr 26, 2019 - Python
3D coronal mass ejection flux rope modeling
Grad-Shafranov reconstruction for interplanetary magnetic flux ropes
We identify and visualize time windows where the moon is exposed to the solar wind radiation environment outside the magnetotail. This information was used to select experimental time periods for the Deep Space Radiation Genomics (DSRG) experiment on Artemis 1.
Classic time-elongation fitting for heliospheric imager data
Data Analysis as part of my Senior Sophistor Research Project
Python code to produce Parker's like solar wind modeling (isopoly) including expansion factor effects, and streamline tracing.
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