Research Highlights

Research Highlights

A selection of highlights culled from publications by HAO staff.

Impact of increasing greenhouse gases on the ionosphere and thermosphere

Impact of increasing greenhouse gases on the ionosphere and thermosphere response to a May 2024-like geomagnetic superstorm

N. M. Pedatella, H. Liu, H.-L. Liu, A. Herrington, and J. McInerney focus on understanding how changes in the background state of the upper atmosphere due to increases in CO2 alter the response of the ionosphere and thermosphere to geomagnetic storms finding that increasing levels of CO2 generally result in a weaker response of the ionosphere and thermosphere to geomagnetic storms in absolute terms, while their relative responses enhance at higher CO2 levels.

interhemisphere coupling simulated by WACCM6

Seasonal and Interannual Variation of the Interhemispheric Coupling during the Austral Winter in WACCM6

Dai Koshin, Nick Pedatella, and Anne Smith describe the coupling between the winter stratosphere in the Southern Hemisphere and the northern upper mesosphere as seen in a long-term whole atmosphere model simulation revealing interannual variation is associated with the phase of the intraseasonal oscillation in the equatorial mesosphere and lower thermosphere.

Global-scale toroid patterns

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

Mausumi Dikpati, Marianna B. Korsos, Aimee A. Norton, Breno Raphaldini, Kiran Jain, Scott W. McIntosh, Peter A. Gilman, Andre S. W. Teruya and Nour E. Raouafi analyzed active region (AR) 13664 during a superactive emergence event. They conclude that this superstorm was caused by enhanced magnetic complexity occurring due to intricate interactions among multiple active regions emerging at nearly the same locations. 

multifluid MAGE application

Multifluid equations for MHD

J. G. Lyon, V. G. Merkin, K. A. Sorathia, and M. J. Wiltberger describe a multifluid approach to observing ionized atoms in near-Earth space showing how changes in the magnetic field direction can act to accelerate ions along the field, and modeling how plasma waves behave in such a multifluid environment. They present results of a super-computer simulation of the near-Earth space, modeling the behavior of different plasma fluids and their interactions during a geomagnetic storm.

comparison between AI-enhanced images and high-quality reference data

A deep learning framework for instrument-to-instrument translation of solar observation data

R. Jarolim, A. M. Veronig, W. Pötzi, and T. Podladchikova recently developed a new deep learning framework for Instrument-To-Instrument translation of solar observation data, enabling homogenized data series across multi-instrument datasets. The study demonstrates that the available data sets can directly profit from instrumental improvements, by applying the method to four different applications of ground- and space-based solar observations. 

sample of 650 PhD theses used in the study

Changing methodologies in solar physics

Philip Judge:  For the first time, the methods in solar physics are reviewed using statistical methods. This study attempts to establish a basis for understanding how methods used in research in solar physics have evolved since WWII.

MAGE simulation and ICON observation of zonal thermospheric winds and ion drifts

Penetrating electric field with/without disturbed electric fields During the 7-8 July 2022 geomagnetic storm simulated by MAGE and observed by ICON MIGHTI

Qian Wu, Dong Lin, Wenbin Wang, Kevin Pham, Liying Qian, Haonan Wu, Thomas J. Immel, and Erdal Yigit, using a numerical model, simulated the nighttime ionospheric disturbances caused by electric fields that enter this system from the magnetosphere and electric fields generated internally by changes in the thermospheric winds.

Observed Neutral Winds

Effects of High-Latitude Input on Neutral Wind Structure and Forcing During the 17 March 2013 Storm

Katherine Davidson, Gang Lu, Mark Conde present a quantitative assessment of the thermospheric forcing and its dependence on high-latitude driving. Due to its coupling with the ionosphere via ion-neutral collisions, the simulated neutral wind and the corresponding thermospheric forcing from Global Circulation Models (GCMs) are highly dependent on the model's high-latitude ionospheric input. 

Averaged mass density

Evaluating F10.7 and F30 radio fluxes as long-term solar proxies of energy deposition in the thermosphere

Liying Qian, and Kalevi Mursula use model simulations and observations to examine how well the F10.7 and F30 solar radio fluxes have represented solar forcing in the thermosphere during the last 60 years of weakening solar activity.