Results 161 to 170 of about 47,350 (264)
A TIEGCM-based inversion model for ionosphere-thermosphere parameters driven by three-dimensional electron density. [PDF]
Chen Z +6 more
europepmc +1 more source
Abstract Doppler frequency shifts (DFSs) recorded by continuous wave‐high frequency Doppler sounding systems and ionograms observed by five ionosondes in Taiwan and Japan are used to study three‐dimensionally seismo‐ and tsunami‐traveling ionospheric disturbances (STIDs and TTIDs) triggered by the 29 July 2025 Mw8.8 Kamchatka earthquake.
Yao‐Chun Chen +9 more
wiley +1 more source
The Ringed World: Saturn from Cassini to The James Webb Space Telescope. [PDF]
Tiranti P.
europepmc +1 more source
HF Heating Effects as Seen From Below and Above: First Results of Joint SURA–Ionosfera‐M Experiment
Abstract This paper presents the first results of a coordinated experiment on the ionospheric plasma response to high‐frequency (HF) overdense heating, conducted using the SURA heating facility and the Ionosfera‐M satellite. The experiment combined ground‐based observations with in situ satellite measurements, enabling a comprehensive study of ...
A. A. Chernyshov +18 more
wiley +1 more source
Adaptive station selection incorporating observation data quality for UPD estimation. [PDF]
Gu S +5 more
europepmc +1 more source
Abstract The solar quiet (Sq) current and equatorial electrojet are widely known as one of the fundamental currents in ionosphere. Although the Sq‐EEJ current system has been extensively investigated, the manner in which Hall and Pedersen current components collectively organize the system has not been clearly described.
T. Ijuin, H. Jin, A. Yoshikawa
wiley +1 more source
Mars' induced magnetosphere can form under radial interplanetary magnetic field. [PDF]
Lin R +16 more
europepmc +1 more source
Abstract Electron and proton precipitation into the nightside ionosphere is a key process in magnetosphere–ionosphere coupling. Although auroral electron precipitation at ∼0.1 ${\sim} 0.1$–10 keV is traditionally considered the main driver of auroral emissions, recent studies show that >30 ${ >} 30$ keV electrons and protons can significantly ...
S. R. Kamaletdinov +22 more
wiley +1 more source
Jupiter's brightest auroras are powered by locally generated Alfvén waves. [PDF]
Sulaiman AH +12 more
europepmc +1 more source
Abstract We investigate the nighttime equatorial ionosphere during the 19 January 2026 geomagnetic storm using Global‐scale Observations of the Limb and Disk OI 135.6 nm observations and ground‐based GPS Total Electron Content. The observations reveal a pronounced longitudinal asymmetry in the post‐sunset equatorial ionization anomaly (EIA).
Deepak K. Karan +6 more
wiley +1 more source

