Results 1 to 10 of about 835 (185)

Modeling the evolution of chorus waves into plasmaspheric hiss [PDF]

open access: yesJournal of Geophysical Research, 2011
Plasmaspheric hiss (PH) is a band-limited, incoherent whistler mode emission found predominantly in the plasmasphere or high-density plasma regions in the near-Earth space environment.
Bortnik, J.   +4 more
core   +5 more sources

Effect of plasma density on diffusion rates due to wave particle interactions with chorus and plasmaspheric hiss: extreme event analysis [PDF]

open access: yesAnnales Geophysicae, 2014
Wave particle interactions play an important role in controlling the dynamics of the radiation belts. The purpose of this study is to estimate how variations in the plasma density can affect diffusion rates resulting from interactions between chorus ...
A. Sicard-Piet   +4 more
doaj   +6 more sources

Exohiss wave enhancement following substorm electron injection in the dayside magnetosphere [PDF]

open access: yesEarth and Planetary Physics, 2018
Exohiss is a low-frequency structureless whistler-mode emission potentially contributing to the precipitation loss of radiation belt electrons outside the plasmasphere.
ZhongLei Gao   +10 more
doaj   +2 more sources

A first approach to model the low-frequency wave activity in the plasmasphere [PDF]

open access: yesAnnales Geophysicae, 2002
A comprehensive empirical model of waves is developed in the objective to simulate wave-particle interactions involved in the loss and acceleration of radiation belt electrons.
R. André   +5 more
doaj   +5 more sources

Analysis of plasmaspheric hiss wave amplitudes inferred from low-altitude POES electron data: Technique sensitivity analysis [PDF]

open access: yesJournal of Geophysical Research: Space Physics, 2015
A novel technique capable of inferring wave amplitudes from low-altitude electron measurements from the Polar Operational Environmental Satellites (POES) spacecraft has been previously proposed to construct a global dynamic model of chorus and ...
Blake, J. B.   +12 more
core   +7 more sources

Wave-induced loss of ultra-relativistic electrons in the Van Allen radiation belts. [PDF]

open access: yesNat Commun, 2016
The dipole configuration of the Earth's magnetic field allows for the trapping of highly energetic particles, which form the radiation belts. Although significant advances have been made in understanding the acceleration mechanisms in the radiation belts,
Shprits YY   +12 more
europepmc   +3 more sources

Deep learning model of hiss waves in the plasmasphere and plumes and their effects on radiation belt electrons

open access: yesFrontiers in Astronomy and Space Sciences, 2023
Hiss waves play an important role in removing energetic electrons from Earth’s radiation belts by precipitating them into the upper atmosphere. Compared to plasmaspheric hiss that has been studied extensively, the evolution and effects of plume hiss are ...
Sheng Huang   +11 more
doaj   +2 more sources

On How High-Latitude Chorus Waves Tip the Balance Between Acceleration and Loss of Relativistic Electrons. [PDF]

open access: yesGeophys Res Lett, 2019
Modeling and observations have shown that energy diffusion by chorus waves is an important source of acceleration of electrons to relativistic energies.
Wang D, Shprits YY.
europepmc   +3 more sources

Cross Correlation Between Plasmaspheric Hiss Waves and Enhanced Radiation Levels at Aviation Altitudes

open access: yesSpace Weather
Enhanced radiation in the Earth's atmosphere can pose serious hazards to pilots, aircraft passengers, and commercial space travelers. Recent results have shown, statistically, that there is a strong correlation between dose rates observed by Automated ...
Homayon Aryan   +5 more
doaj   +2 more sources

Multi‐Parameter Chorus and Plasmaspheric Hiss Wave Models [PDF]

open access: yesJournal of Geophysical Research: Space Physics, 2020
AbstractThe resonant interaction of energetic particles with plasma waves, such as chorus and plasmaspheric hiss waves, plays a direct and crucial role in the acceleration and loss of radiation belt electrons that ultimately affect the dynamics of the radiation belts.
Homayon Aryan   +5 more
openaire   +4 more sources

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