Results 61 to 70 of about 2,907 (207)
A quantitative model for cyclotron wave-particle interactions at the plasmapause [PDF]
The formation of a zone of energetic electron precipitation by the plasmapause, a region of enhanced plasma density, following energetic particle injection during a magnetic storm, is analyzed.
D. L. Pasmanik +8 more
doaj +1 more source
Abstract Field‐line curvature scattering (FLCS) is believed to be the primary mechanism forming electron isotropy boundaries (IB) and can rapidly scatter relativistic electrons from the outer radiation belt. However, its direct and quantitative impact on controlling outer belt electron lifetimes has never been directly assessed.
Man Hua +17 more
wiley +1 more source
A Predictive Model of the Position of Plasmapause Based on Lunar Phase and Deep Learning Framework
The plasmapause position is crucial for understanding magnetospheric dynamics and space weather forecasting. This study pioneers the integration of lunar phase (LP) into plasmapause modeling using two neural network architectures (BP and fully connected ...
Yajun Li +11 more
doaj +1 more source
Guiding of whistler-mode waves with frequencies above one half of the gyrofrequency in the magnetosphere [PDF]
Ray-tracing calculations show that a trough, L = 4.6, located in the region outside the plasmapause is capable to guide whistler-mode waves in frequency range 0.5fBmin−0.64fBmin, from one hemisphere to the other.
Šulić D.M.
doaj +1 more source
Plasmapause Disturbances Synchronized with Magnetospheric Disturbances.
Quasi pulsive depleting plasma density variations with period ranging from a few to a few tens sec with depletion up to 30 to 50% of the ambient non-depleted plasmapause density have been observed in the occasion of the plasmapause crossing by the Akebono (EXOS-D) satellite, in association with the enhancements of the local upper hybrid mode plasma ...
Akira Morioka, Hiroshi Oya
openaire +2 more sources
Abstract Energetic electron precipitation plays a pivotal role in shaping Earth's radiation belt dynamics and drives significant physical and chemical changes in the upper atmosphere. However, the detailed mechanisms governing the loss of relativistic electrons have remained unclear, largely due to the limited energy coverage and coarse resolution of ...
Zheng Xiang +13 more
wiley +1 more source
Abstract The 1–100 keV electron precipitation during storm time has been studied by applying the updated ELSPEC inversion method to field‐aligned electron density profiles measured by the EISCAT Tromsø radar at L = 6.5. The statistical properties of peak energy, total energy flux, and total number flux as a function of MLT have been studied for the two
N. M. Ellahouny +6 more
wiley +1 more source
Abstract Whistler‐mode chorus waves play a key role in driving radiation belt dynamics by enabling both acceleration of electrons to relativistic energies as well as their loss into the atmosphere via pitch‐angle scattering. The ratio between the electron plasma frequency (fpe ${f}_{pe}$) and the electron gyrofrequency (fce ${f}_{ce}$) significantly ...
K. A. Bunting +5 more
wiley +1 more source
Guiding Medium Radio Waves in the Magnetosphere: Features and Geophysical Conditions
We present experimental results related to the features and geophysical conditions for the occurrence of the long-delay echo (LDE) signals in the medium-wave (MW) frequency range observed on 20 January 2025, at the Gor’kovskaya observatory near St ...
Alexey S. Kalishin +5 more
doaj +1 more source
The Real‐Time Advanced Ionospheric Data Assimilation (AIDA) Model
Abstract The Advanced Ionospheric Data Assimilation (AIDA) is a real‐time data assimilation model of global 3D ionosphere and plasmasphere electron density. Changes in the local space environment can occur on very short timescales, particularly during disturbed geomagnetic conditions.
Benjamin Reid +5 more
wiley +1 more source

