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Neutron Transport and Layer-Resolved Radiation Effects in Potassium-Ion Cells with Organic and Inorganic Cathodes Under Space-Relevant Irradiation. [PDF]
Nanomaterials (Basel)Novoselov IE, Zhidkov IS.
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Simulating 135 years of post-hatchling sea turtle dispersal in a dynamic North Atlantic Ocean. [PDF]
Sci RepArendt MD, Putman NF.
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Space Science Reviews, 2000
The emission of energetic particles from the Sun is one of the major manifestations of high energy astrophysics and is related to a variety of astrophysical and geophysical phenomena in the heliosphere. An event of solar energetic particles (SEP) is seen as a sudden rise of the counting rate of the background galactic cosmic rays reaching a high value ...
Ryan JM
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The emission of energetic particles from the Sun is one of the major manifestations of high energy astrophysics and is related to a variety of astrophysical and geophysical phenomena in the heliosphere. An event of solar energetic particles (SEP) is seen as a sudden rise of the counting rate of the background galactic cosmic rays reaching a high value ...
Ryan JM
exaly +3 more sources
Solar flares and energetic particles [PDF]
Philosophical Transactions Series A, Mathematical, Physical, and Engineering Sciences, 2012 Solar flares are now observed at all wavelengths from γ -rays to decametre radio waves. They are commonly associated with efficient production of energetic particles at all energies. These particles play a major role in the active Sun because they contain a large amount of the energy released
Vilmer Nicole
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Solar Energetic Particle Isotopic Composition
Space Science Reviews, 1998We discuss isotopic abundance measurements of heavy (6 ≤ Z ≤ 14) solar energetic particles with energies from ∼15 to 70 MeV/nucleon, focusing on new measurements made on SAMPEX during two large solar particle events in late 1992. These measurements are corrected for charge/mass dependent acceleration effects to obtain estimates of coronal isotopic ...
Edward C. Stone, R A Leske, E C Stone
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2021
Solar energetic particles (SEPs) have been studied for over seven decades, initially from ground-based instrumentation and now routinely from spacecraft throughout the heliosphere. Our knowledge of the acceleration and transport of these particles from close to the Sun througzh the interplanetary medium has advanced dramatically in the last 40 years as
Cohen, Christina M. S. +4 more
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Solar energetic particles (SEPs) have been studied for over seven decades, initially from ground-based instrumentation and now routinely from spacecraft throughout the heliosphere. Our knowledge of the acceleration and transport of these particles from close to the Sun througzh the interplanetary medium has advanced dramatically in the last 40 years as
Cohen, Christina M. S. +4 more
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Large gradual solar energetic particle events
Living Reviews in Solar Physics, 2016 Solar energetic particles, or SEPs, from suprathermal (few keV) up to relativistic ( ∼ few GeV) energies are accelerated near the Sun in at least two ways: (1) by magnetic reconnection-driven processes during solar flares resulting in impulsive SEPs, and (2) at fast coronal-mass-ejection-driven shock waves that produce large gradual SEP events.
Mihir I Desai, Joe Giacalone
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Solar wind turbulence: Connections with energetic particles
New Astronomy, 2021Abstract For the solar wind, a wealth of observational evidence indicates that turbulence is an important dynamical process for velocity (v), magnetic (b), and other related fluctuations at MHD (fluid) scales. Here we review such observations and turbulence features, including discussion of when wave or turbulence descriptions can (or cannot) explain
Oughton, Sean, Engelbrecht, N. Eugene
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