Unprecedented extreme depletion of Earth's ionosphere during the May 2024 super geomagnetic storm revealed by the Chinese Meridian Project. [PDF]
Cao J.
europepmc +1 more source
Uranus' Long‐Term Thermospheric Cooling Is Unlikely to Be Primarily Driven by the Solar Wind
Abstract Over the last 40 yrs, Uranus' thermospheric temperature has decreased by ∼8 K/yr. Here we show that this is less likely to be driven by solar wind kinetic power than previously thought. We determine that the solar wind kinetic power at Uranus has been increasing since the start of solar cycle 24 in 2009, while Uranus's thermospheric ...
Jamie M. Jasinski +5 more
wiley +1 more source
A High-Precision Ionospheric Channel Estimation Method Based on Oblique Projection and Double-Space Decomposition. [PDF]
Wei Z, Guo B, Li Z, Zhou Q.
europepmc +1 more source
Abstract Low‐altitude measurements of energetic electron fluxes offer insight into the dynamics of the radiation belts and plasma sheet. However, distinguishing between key magnetospheric regions–such as inner belt, slot region, outer belt, and plasma sheet–based on low‐altitude data remains challenging, particularly for missions lacking pitch‐angle ...
Weiqin Sun +7 more
wiley +1 more source
Evidence for Alfvén waves powering auroral arc via a static electric potential drop. [PDF]
Tian S +10 more
europepmc +1 more source
Automated Ionospheric Scattering Layer Hypothesis Generation for Detected and Classified Auroral Global Positioning System Scintillation Events [PDF]
Vaishnavi Sreenivash +2 more
openalex +1 more source
The Global Propagation of Hiss Waves Originating From Dynamic Plasmaspheric Plume
Abstract Hiss waves play a critical role in shaping Earth's radiation belts and mediating magnetosphere‐ionosphere energy transfer. Intense hiss emissions are frequently generated within dynamic plasmaspheric plumes through linear and nonlinear wave‐particle interactions.
Xiangling Ding +6 more
wiley +1 more source
A case study of the three-dimensional co-seismic ionospheric disturbance evolution. [PDF]
Song R +4 more
europepmc +1 more source
Plasma Acceleration by Magnetic Tension Forces in the Martian Magnetotail: MAVEN Observations
Abstract The Martian magnetotail is a dynamic region where several processes contribute to plasma acceleration. Here, we analyze ∼5 ${\sim} 5$ years of Mars Atmosphere and Volatile EvolutioN (MAVEN) data to evaluate the role of magnetic tension forces in driving plasma acceleration within current sheets in the tail. Based on magnetic field measurements,
Norberto Romanelli +15 more
wiley +1 more source

