2024 THEMIS SCIENCE NUGGETS

SUMMARIES OF THEMIS RESEARCH

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Adetayo Victor Eyelade, July 2024
The Response of the Earth Magnetosphere to Changes in the Solar Wind Dynamic Pressure: I. Ion and Electron Kappa Distribution Functions.

We analyze data from the five THEMIS satellites to investigate these changes. We focus on the kappa-index for ions and electrons to better understand their behavior and what they reveal about plasma environments, such as the Earth’s magnetosphere. Read more.



Anton Artemyev, July 2024
The Response of the Earth Magnetosphere to Changes in the Solar Wind Dynamic Pressure: I. Ion and Electron Kappa Distribution Functions.

Energetic particle precipitation may significantly alter the physics of magnetosphere-ionosphere coupling within SAPS. Relativistic electrons will extend the altitude range of ionization enhancement to <100 km, while energetic ion precipitation will extend its latitudinal range. We study energetic particle precipitation during SAPS using observations from the low-altitude ELFIN CubeSats in conjugation with near-equatorial THEMIS measurements. Read more.



Anton Artemyev, August 2024
The Response of the Earth Magnetosphere to Changes in the Solar Wind Dynamic Pressure: I. Ion and Electron Kappa Distribution Functions.

During strong substorms, energetic electrons can be transported deep into the inner magnetosphere, reaching the slot region or even smaller L-shells. This transport is usually too fast to be explained by radial diffusion. Read more.



Terry Z. Liu, September 2024
Global Observations of Geomagnetically Induced Currents Caused by an Extremely Intense Density Pulse During a Coronal Mass Ejection

Geomagnetically induced currents (GIC) in power systems are among the most severe space weather hazards, yet the mechanisms driving large GIC events are not well understood... Read more.



Xiangxi Deng and Zhigang Yuan , September 2024
THEMIS Probes Observed Temporal Evolution of Electron Accelerations behind the Dipolarization Front in the Earthʼs Magnetotail

The dipolarization front (DF), as the leading edge of fast earthward plasma flow in the planetary magnetotail, plays an important role in the plasma energization and energy transportation from the magnetotail to inner magnetosphere. Read more.






Please send comments/suggestions to
Emmanuel Masongsong / emasongsong @ igpp.ucla.edu