Sushant S. Mahajan
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Spectral Methods for 3D Solar Dynamo simulations
Calibration of automatic detection of Solar Filaments
Torsional Oscillations and the Solar Cycle: the Waldmeier effect
Surface Flux Transport Simulation
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mahajan(at)astro.gsu.edu
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515, Kell Hall
, Atlanta, GA
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Homepage
Research
Datasets
>
SWAN
Spectral Methods for 3D Solar Dynamo simulations
Calibration of automatic detection of Solar Filaments
Torsional Oscillations and the Solar Cycle: the Waldmeier effect
Surface Flux Transport Simulation
Publications
Teaching
Astronomy Labs
Bash tutorial for beginners
Outreach
Blog
Contact
New Page
New Page
