70th EAGE Conference and Exhibition Incorporating SPE EUROPEC 2008 2008
DOI: 10.3997/2214-4609.20147669
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3D Exploration for Remaining Oil Using Historical Production Data

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“…Electron measurements from the 3D Plasma and Energetic Particle instrument on the WIND spacecraft near 1 AU find a superthermal component of the solar wind electron population at energies above ∼2 keV, denoted the "superhalo", with a power-law (f (E) ∼ E −δ with δ ∼ 2.5) spectrum extending to >100 keV, and a nearly isotropic angular distribution (Lin 1997(Lin , 1998. Superhalo electrons appear to be the electron counterpart of the power-law-tail suprathermal ions above solar wind 2 NUMERICAL METHOD…”
Section: Introductionmentioning
confidence: 99%
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“…Electron measurements from the 3D Plasma and Energetic Particle instrument on the WIND spacecraft near 1 AU find a superthermal component of the solar wind electron population at energies above ∼2 keV, denoted the "superhalo", with a power-law (f (E) ∼ E −δ with δ ∼ 2.5) spectrum extending to >100 keV, and a nearly isotropic angular distribution (Lin 1997(Lin , 1998. Superhalo electrons appear to be the electron counterpart of the power-law-tail suprathermal ions above solar wind 2 NUMERICAL METHOD…”
Section: Introductionmentioning
confidence: 99%
“…L.-P. Yang et al nearly isotropic angular distribution (Lin 1997(Lin , 1998. Superhalo electrons appear to be the electron counterpart of the power-law-tail suprathermal ions above solar wind and pickup ion energies that are observed throughout the heliosphere at all the times (e.g., Gloeckler et al 2008;Wimmer-Schweingruber et al 2013).…”
mentioning
confidence: 99%