Electron energy partition across interplanetary shocks: II. Statistics
arXiv:1909.09050 · doi:10.3847/1538-4365/ab5445
Abstract
A statistical analysis of 15,210 electron velocity distribution function (VDF) fits, observed within 2 hours of 52 interplanetary (IP) shocks by the spacecraft near 1 AU, is presented. This is the second in a three-part series on electron VDFs near IP shocks. The electron velocity moment statistics for the dense, low energy core, tenuous, hot halo, and field-aligned beam/strahl are a statistically significant list of values illustrated with both histograms and tabular lists for reference and baselines in future work. The beam/strahl fit results in the upstream are currently the closest thing to a proper parameterization of the beam/strahl electron velocity moments in the ambient solar wind. This work will also serve as a 1 AU baseline and reference for missions like and . The median density, temperature, beta, and temperature anisotropy values for the core(halo)[beam/strahl] components, with subscripts ()[], of all fit results respectively are 11.3(0.36)[0.17] , 14.6(48.4)[40.2] , 0.93(0.11)[0.05], and 0.98(1.03)[0.93]. The nuanced details of the fitting method and data product description were published in Paper I and the detailed analysis of the results will be shown in Paper III.
40 pages, 11 figures, 18 tables, to be submitted to Astrophys. J. Suppl
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Cited by in corpus (19)
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