Liu Fe xiii 10747 line and CME eruption
Mar 3, 2023

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

SAMI3 simulation results for electron denisity
Oct 5, 2022

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

3 Scatter density plots of the retrieved value of Blos
Sep 23, 2022

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

Lower-atmosphere processes in the ionosphere-thermosphere
Sep 16, 2022

Scientific Motivations and Future Directions of Whole Atmosphere Modeling

Daily averaged TEC
Sep 2, 2022

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

Center for Geospace Storms: Transforming the understanding and predictability of space weather
Jul 11, 2022

The Multiscale Atmosphere-Geospace Environment (MAGE) model

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
Jul 11, 2022

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

Comparisons of local time structure of molecular oxygen at 21°N, 170 km altitude
Jul 11, 2022

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

Snapshot from a two-dimensional test simulation setup with a 8x8Mm domain reaching from the upper convection zone into the transition region
Mar 3, 2022

Efficient numerical treatment of ambipolar and Hall drift as hyperbolic system

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)
Mar 3, 2022

On the (In)stability of Sunspots

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