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- W2059848810 abstract "A theoretical model of weak electron phase-space holes is used to interpret bipolar field structures observed in space. In the limit $e{ensuremath{phi}}_{mathrm{max}}/{T}_{e}ensuremath{ll}1$ the potential of the structure has the unique form, $ensuremath{phi}(x)={ensuremath{phi}}_{mathrm{max}}{mathrm{sech}}^{4}(x/ensuremath{alpha})$, where ${ensuremath{phi}}_{mathrm{max}}$ depends on the derivative of the trapped distribution at the separatrix, while $ensuremath{alpha}$ depends only on a screening integral over the untrapped distribution. Idealized trapped and passing electron distributions are inferred from the speed, amplitude, and shape of satellite waveform measurements of weak bipolar field structures." @default.
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- W2059848810 date "2007-10-05" @default.
- W2059848810 modified "2023-09-23" @default.
- W2059848810 title "Theory of Weak Bipolar Fields and Electron Holes with Applications to Space Plasmas" @default.
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- W2059848810 doi "https://doi.org/10.1103/physrevlett.99.145002" @default.
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