MHD | High Altitude Observatory

Magnetohydrodynamics

The Coronal Veil

3D view of the simulated corona; bottom panel: magnetogram; back panel: synthetic AIA 211A coronal image; middle vertical plane: volumetric emissivity. Field lines are included for reference.

Acoustic-gravity wave propagation characteristics in three-dimensional radiation hydrodynamic simulations of the solar atmosphere

ν − z phase diagrams (cuts at constant horizontal wavenumber at approx. 2 and 4 Mm−1 through the stacks of the layer-by-layer two-dimensional k − ω phase difference diagrams) for various MURaM models

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Mausumi Dikpati

Space Weather Challenge & Forecasting Implications Of Rossby Waves

Rossby waves

Physics Of MHD Rossby Waves In The Sun

Retrograde and prograde Rossby waves

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