Mausumi Dikpati | High Altitude Observatory

A Multi-layer Magnetohydrodynamic Shallow-water Model of The Solar Tachocline: Equilibrium Shape and Thickness

Spherical views of tachocline shapes

MHD-tachocline-model solutions of magnetic vectors

Warped toroid patterns and MHD-tachocline-model solutions of magnetic vectors

Analysis Of Short-term Solar Activity Variability and Estimating Timings of Next Enhanced Bursts

Zoomed-in burst-envelope forecasts from January 2024 to April 2026

HAO research featured on AAS Nova

Mother’s Day Superstorms

Mother's Day Superstorms: Pre- and Post-storm Evolutionary Patterns of AR 13664/8

Global-scale toroid patterns

A Magnetohydrodynamic Mechanism for the Formation of Solar Polar Vortices

Simulation of an evolving polar vortex

Spectra of solar shallow-water waves from bright point observations

Hovmoller (time × longitude) diagram at 30◦ latitudes

Evolution Of Amplitude And Longitude Phase Of Tachocline Rossby Waves Diffusing To The Photosphere

Rosby Wave penetration

Global and Local Dynamics of X-flare Producing Active Regions During Solar Cycle 25 Peak-Phase

21st February 2024 synoptic map

Exploring Spatial and Temporal Patterns in the Debrecen Solar Faculae Database

Scenario of the faculae distribution

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