modeling | High Altitude Observatory

Magnetic field and plasma diagnostics for solar coronal mass ejections: A case study using the forward modeling approach

Liu Fe xiii 10747 line and CME eruption

Equinoctial Asymmetry in the Upper Ionosphere: Comparison of Satellite Observations and Models

SAMI3 simulation results for electron denisity

Effects of spectral resolution on simple magnetic field diagnostics of the Mg II h & k lines

3 Scatter density plots of the retrieved value of Blos

Scientific Motivations and Future Directions of Whole Atmosphere Modeling

Lower-atmosphere processes in the ionosphere-thermosphere

On the variability of total electron content over Europe during the 2009 and 2019 Northern Hemisphere SSWs

Daily averaged TEC

The Multiscale Atmosphere-Geospace Environment (MAGE) model

Center for Geospace Storms: Transforming the understanding and predictability of space weather

The effects of IMF By on the middle thermosphere during a geomagnetically “quiet” period at solar minimum

The polar view of the percentage difference of simulated ∑O/N2 and GOLD observed ∑O/N2 between DOY 111 and 110 at 15:10 UT in 2019. The perimeter latitude is 30°N

The Molecular Oxygen Density Structure of the Lower Thermosphere as Seen by GOLD and Models

Comparisons of local time structure of molecular oxygen at 21°N, 170 km altitude

Efficient numerical treatment of ambipolar and Hall drift as hyperbolic system

Snapshot from a two-dimensional test simulation setup with a 8x8Mm domain reaching from the upper convection zone into the transition region

On the (In)stability of Sunspots

Maps of the magnetic field strength at depth of z = −7.5 Mm beneath the solar photosphere at different times (indicated in red in each panel)

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