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Particle Diffusion in the Radiation Belts

More information about this seller Contact this seller 4. Condition: Used: Very Good. Seller Inventory Y More information about this seller Contact this seller 5. From: Antiquariat am St. Physics and chemistry in space 7. IX, S. Sprache: Englisch, gutes Exemplar. More information about this seller Contact this seller 6. Item added to your basket View basket. Proceed to Basket. View basket. Continue shopping. Title: particle diffusion radiation belts. The relativistic electron-proton telescope REPT instrument on board the radiation belt storm probes RBSP spacecraft: Characterization of Earth's radiation belt high-energy particle populations.

Blake, J. Spence, H. Wygant, J. The electric field and waves instruments on the radiation belt storm probes mission. Kletzing, C. McIlwain, C.

Coordinates for mapping the distribution of magnetically trapped particles. Southwood, D. Charged particle behavior in low-frequency geomagnetic pulsations. II - Graphical approach. Zong, Q. Ultralow frequency modulation of energetic particles in the dayside magnetosphere. Claudepierre, S. Van Allen Probes observation of localized drift resonance between poloidal mode ultra-low frequency waves and 60 keV electrons.


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Torrence, C. A practical guide to wavelet analysis. Mann, I. Discovery of the action of a geophysical synchrotron in the Earth's Van Allen radiation belts. Tu, W. Quantifying radial diffusion coefficients of radiation belt electrons based on global MHD simulation and spacecraft measurements. Green, J. Relativistic electrons in the outer radiation belt: differentiating between acceleration mechanisms. Chen, Y. The energization of relativistic electrons in the outer Van Allen radiation belt.

Su, Z. Brautigam, D. CRRES electric field power spectra and radial diffusion coefficients. Huang, C. Modeling radiation belt radial diffusion in ULF wave fields: 1.

Physics and Chemistry in Space Vol 7: Particle Diffusion in the Radiation Belts - IOPscience

Ozeke, L. ULF wave derived radiation belt radial diffusion coefficients. Rae, I. Ground-based magnetometer determination of in situ Pc ULF electric field wave spectra as a function of solar wind speed. Ali, A. Magnetic field power spectra and magnetic radial diffusion coefficients using CRRES magnetometer data.

Takahashi, K. Meredith, N. Substorm dependence of chorus amplitudes: Implications for the acceleration of electrons to relativistic energies.

References

Model of the energization of outer-zone electrons by whistler-mode chorus during the October 9, geomagnetic storm. Timescale for radiation belt electron acceleration by whistler mode chorus waves. Refilling of the slot region between the inner and outer electron radiation belts during geomagnetic storms. Li, W. Global model of lower band and upper band chorus from multiple satellite observations. A new diffusion matrix for whistler mode chorus waves. Nonstorm time dynamics of electron radiation belts observed by the Van Allen Probes.

Intense duskside lower band chorus waves observed by Van Allen Probes: Generation and potential acceleration effect on radiation belt electrons. Xiao, F. Wave-driven butterfly distribution of Van Allen belt relativistic electrons.


  1. The Devils Cave (Bruno, Chief of Police, Book 5).
  2. Wave driven diffusion in radiation belt dynamics.
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  6. Albert, J. Three-dimensional diffusion simulation of outer radiation belt electrons during the october 9, , magnetic storm. Evolution of electron fluxes in the outer radiation belt computed with the VERB code. Radiation belt electron dynamics driven by adiabatic transport, radial diffusion, and wave-particle interactions.

    Ion flux oscillations associated with a radially polarized transverse Pc 5 magnetic pulsation. Kurth, W. Electron densities inferred from plasma wave spectra obtained by the Waves instrument on Van Allen Probes. Tsyganenko, N.

    Modeling the dynamics of the inner magnetosphere during strong geomagnetic storms. Download references. King, N. Papatashvilli and CDAWeb for providing interplanetary parameters and magnetospheric indices, and acknowledge C. Torrence and G. Compo for providing the wavelet analysis software. Correspondence to Zhenpeng Su. This work is licensed under a Creative Commons Attribution 4. Reprints and Permissions. Journal of Geophysical Research: Space Physics Geophysical Research Letters Journal of Atmospheric and Solar-Terrestrial Physics By submitting a comment you agree to abide by our Terms and Community Guidelines.

    Particle Diffusion in the Radiation Belts

    If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate. Advanced search. Skip to main content. Subjects Particle astrophysics. Abstract Van Allen radiation belts are typically two zones of energetic particles encircling the Earth separated by the slot region. Introduction The geomagnetic field geometry allows three quasi-periodic motions of outer Van Allen radiation belt 1 relativistic electrons over distinct timescales: gyration about the magnetic field line on a timescale of milliseconds; bounce along the magnetic field line between two magnetic mirror points on a timescale of seconds; drift circling the Earth on a timescale of kiloseconds.

    Figure 1: An overview of the 15 February radiation belt event. Full size image. Figure 2: Electromagnetic power spectral densities of high-frequency and very-low-frequency waves. Figure 3: Relative wavelet power of residual electron fluxes. The advent of artificial earth satellites in opened a new dimension in the field of geophysical exploration. Discovery of the earth's radiation belts, consisting of energetic electrons and ions chiefly protons trapped by the geomagnetic field, followed almost immediately [1,2]' This largely unexpected development spurred a continuing interest in magnetospheric exploration, which so far has led to the launching of several hundred carefully instrumented spacecraft.

    Since their discovery, the radiation belts have been a subject of intensive theoretical analysis also.

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    The underlying kinematical framework of radiation-belt theory is given by the adiabatic theory of charged-particle motion [3J, and the interesting dynamical phenomena are associated with the violation of one or more of the kinematical invariants of adiabatic motion. Among the most important of the operative dynamical processes are those that act in a stochastic manner upon the radiation-belt particles.

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    Such stochastic processes lead to the diffusion of particle distributions with respect to the adiabatic invariants. The observational data indicate that some form of particle diffusion plays an essential role in virtually every aspect of the radiation belts. JavaScript is currently disabled, this site works much better if you enable JavaScript in your browser.