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Found 3 entries in the Bibliography.
Showing entries from 1 through 3
2021 |
The Electron Structure of the Solar Wind Time-series measurements of the number density ncore and temperature Tcore of the core-electron population of the solar wind are examined at 1 AU and at 0.13 AU using measurements from the WIND and Parker Solar Probe spacecraft, respectively. A statistical analysis of the ncore and Tcore measurements at 1 AU finds that the core-electron spatial structure of the solar wind is related to the magnetic-flux-tube structure of the solar wind; this electron structure is characterized by jumps in the values of ncore and Tcore when p ... Borovsky, Joseph; Halekas, Jasper; Whittlesey, Phyllis; Published by: Frontiers in Astronomy and Space Sciences Published on: jun YEAR: 2021   DOI: 10.3389/fspas.2021.690005 Parker Data Used; Solar wind; Heliosphere; interplanetary potential; Corona; Magnetic structure |
2020 |
Nine Outstanding Questions of Solar Wind Physics In situ measurements of the solar wind have been available for almost 60 years, and in that time plasma physics simulation capabilities have commenced and ground-based solar observations have expanded into space-based solar observations. These observations and simulations have yielded an increasingly improved knowledge of fundamental physics and have delivered a remarkable understanding of the solar wind and its complexity. Yet there are longstanding major unsolved questions. Synthesizing inputs from the solar wind research ... Viall, Nicholeen; Borovsky, Joseph; Published by: JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS Published on: 07/2020 YEAR: 2020   DOI: 10.1029/2018JA026005 |
2013 |
Coherent structures, intermittent turbulence, and dissipation in high-temperature plasmas Karimabadi, H.; Roytershteyn, V.; Wan, M.; Matthaeus, W.~H.; Daughton, W.; Wu, P.; Shay, M.; Loring, B.; Borovsky, J.; Leonardis, E.; Chapman, S.~C.; Nakamura, T.~K.~M.; Published by: Physics of Plasmas Published on: 01/2013 YEAR: 2013   DOI: 10.1063/1.4773205 Parker Data Used; astrophysical plasma; plasma Alfven waves; plasma kinetic theory; plasma simulation; plasma temperature; plasma transport processes; plasma turbulence; Solar wind; 52.35.Ra; 94.05.Lk; 94.05.Pt; 52.25.Dg; 52.25.Fi; 52.35.Bj; plasma turbulence; turbulence; Wave/wave wave/particle interactions; Plasma kinetic equations; Transport properties; Magnetohydrodynamic waves |
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