Results 111 to 120 of about 13,800 (221)
The average solar wind in the inner heliosphere: Structures and slow variations [PDF]
Measurements from the HELIOS solar probes indicated that apart from solar activity related disturbances there exist two states of the solar wind which might result from basic differences in the acceleration process: the fast solar wind (v 600 kms(-)1 ...
Schwenn, R.
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The Acceleration of low energy charged particles at interplanetary shock waves
Bibliography: p. 164-173.
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Model for Particles Accelerated at Interplanetary Shocks starting with a Power Law Energy Spectrum
This work is supported by the NSF-REU solar physics program at SAO, grant number AGS-1850750. This work is also partially supported by the NSF under grant 1850774.
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The curvature of the magnetic field plays a crucial role in magnetic confinement, magnetic reconnection, particle heating, and acceleration. Though the magnetic field curvature has been sufficiently investigated in the terrestrial magnetosheath, there is
D. K. Hu +4 more
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Particles accelerated by shocks in the heliosphere [PDF]
The populations of energetic ions accelerated by shocks in the heliosphere are reviewed briefly.
Lee, Martin A.
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Two‐Step Electron Acceleration During a Flux Rope Crossing of Earth's Bow Shock
The generation of cosmic ray particles with ultra‐relativistic energies is a crucial issue in astrophysical and space physics. Shocks have been acknowledged as efficient accelerators in the universe which can produce energetic particles through a variety
D. K. Hu +3 more
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Latitude dependence of co-rotating shock acceleration [PDF]
Energetic particle observations in the outer heliosphere (approx 12 A. U.) by the LECP instruments on the Voyager 1 and Voyager 2 spacecraft are discussed that show a definite latitude dependence of the number and intensity of particle enhancements ...
Gold, R. E. +3 more
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The Polarization Signatures of the Inverse Cascade in Magnetic Turbulence
The inverse cascade of magnetic energy from smaller to larger scales is a key physical process for the formation of coherent magnetic fields in many astronomical turbulent systems.
X. W. Zhu +6 more
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Tempered Superdiffusive Shock Acceleration at a Perpendicular Shock
A theory for steady-state tempered superdiffusive shock acceleration of energetic particles at a plane perpendicular shock is presented that involves solving analytically a tempered fractional Parker transport equation for perpendicular transport in ...
J. A. le Roux, R. K. Shikha
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Particle Acceleration Phenomena in Earth's Magnetosphere and Interplanetary Space
identifier:oai:t2r2.star.titech.ac.jp ...
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