Results 91 to 100 of about 782 (172)
EMIC Wave Distributions Observed by the Van Allen Probes
Characteristics of electromagnetic ion cyclotron (EMIC) waves detected by the Van Allen probes are statistically analyzed, particularly wave-band, bandwidth, and time duration. The Electric and Magnetic Field Instrument Suite and Integrated Science, an instrument on board the Van Allen Probes, provides the necessary magnetic field measurements to ...
openaire +2 more sources
Modeling the EMIC Wave‐Induced Acceleration of Energetic Protons in the Io Footprint Tail
The Io footprint tail (FPT) region is crucial for studying the interactions between Io and Jupiter's magnetosphere. In this region, Juno spacecraft observed significant acceleration of energetic protons, concurrently with electromagnetic ion cyclotron ...
Peng Lu +6 more
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Simultaneous macroscale and microscale wave-ion interaction in near-earth space plasmas. [PDF]
Liu ZY +11 more
europepmc +1 more source
Extreme Energy Spectra of Relativistic Electron Flux in the Outer Radiation Belt. [PDF]
Mourenas D +3 more
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Localized mesospheric ozone destruction corresponding to isolated proton aurora coming from Earth's radiation belt. [PDF]
Ozaki M +10 more
europepmc +1 more source
The wave amplitude is vital for quantifying the impact of electromagnetic ion cyclotron (EMIC) waves on inner magnetospheric dynamics. Previous numerical studies mainly focused on the evolution of total wave energy/amplitude, whose maximum is usually ...
Zuxiang Xue +3 more
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During the May 2024 storm, the minimum Dst index was approximately −412 nT, marking the largest geomagnetic storm of the past decade. This event caused the inner edge of the ring current to penetrate deeply into the inner magnetosphere during the main ...
C.‐W. Jun +15 more
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Pulse Wave Velocity: Is It Time to Reduce the Cutoff Point? [PDF]
Santos-Veloso MAO.
europepmc +1 more source
Mirror Mode Mediated EMIC Wave Generation in the Magnetosheath
Abstract Electromagnetic ion cyclotron (EMIC) waves and mirror modes (MMs), both driven by ion temperature anisotropy, are commonly observed in planetary magnetosheaths. Conventional explanations for their co‐occurrence are largely based on linear instability theory in proton–electron plasmas, which requires comparable growth rates ...
Yifan Wu +5 more
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Low Frequency ULF Waves in the Earth's Inner Magnetosphere: Power Spectra During High Speed Streams and Quiet Solar Wind and Seeding of EMIC Waves. [PDF]
Gamayunov KV, Engebretson MJ.
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