Results 101 to 110 of about 13,753 (202)
Towards advanced forecasting of solar energetic particle events with the PARASOL model
Gradual solar energetic particle (SEP) events are generally attributed to the particle acceleration in shock waves driven by coronal mass ejections (CMEs). Space-weather effects of such events are important, so there has been continuous effort to develop
Afanasiev Alexandr +2 more
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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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Nuclear and ionic charge distribution experiment on ISEE-1 and ISEE-3 [PDF]
The experimental work carried out under this contract is a continuation of that originally performed under Contracts NAS5-20062 and NAS5-26739. The data analyzed are from the Max-Planck Institut/Univ. of Maryland experiment on ISEE-1 and ISEE-3.
Galvin, A. B. +2 more
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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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Predicting the arrival times of solar particles [PDF]
A procedure has been developed to generate a computerized time-intensity profile of the solar proton intensity expected at the earth after the occurrence of a significant solar flare on the sun.
Smart, D. F.
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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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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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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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