solar flare | High Altitude Observatory

AAS Nova Features a Recent Publication by Philip Judge

Images to highlight the corrugated surfaces at which the centers of UV lines are formed (close to τ = 1) in MURaM calculations of the upper solar chromosphere

Responses of the Thermosphere and Ionosphere System to Concurrent Solar Flares and Geomagnetic Storms

The simulated vertical E x B drift velocity (Wi), and the changes of the vertical drift velocity due to the flares, at 300 km and12:00 LT (September 6th – September 11th, 2017)

Measuring the magnetic origins of solar flares, CMEs and Space Weather

A smoothed UV spectrum of α alpha Cen A, obtained by the Hubble Space Telescope

Geospace response to an extreme solar flare

Solar flare effects on magnetospheric convection and ionospheric potential

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