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- W2074006031 abstract "The process of pitch angle scattering by a current sheet is studied using the modified Harris field model. The relationship between the incoming asymptotic pitch angle α in and the outgoing asymptotic pitch angle α out is studied from first principles by numerically integrating the equation of motion. We give evidence that charged particles undergo chaotic scattering by the current sheet. For fixed α in , it is shown that α out exhibits sensitive dependence on the energy parameter Ĥ in certain energy ranges. For fixed Ĥ in the same energy ranges, α out sensitively depends on α in . For other energy values, α out does not show sensitive dependence on α in for most phase angles. The latter energy values occur at the resonance values given by the previously identified relationship Ĥ 1/4 ∼ N + 0.6. Thus α out exhibits no significant sensitivity near these resonance energies. This conclusion applies to a range of α in centered at α in = 0 (i.e., field aligned in the asymptotic region). A distribution of α in is mapped from the asymptotic region to the midplane, and it is found that the resulting particle distribution should have beam structures with well‐collimated pitch angles near each resonance energy value. Implications for the particle distribution functions in the Earth's magnetotail are discussed." @default.
- W2074006031 created "2016-06-24" @default.
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- W2074006031 date "1992-05-01" @default.
- W2074006031 modified "2023-10-16" @default.
- W2074006031 title "Chaotic scattering of pitch angles in the current sheet of the magnetotail" @default.
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- W2074006031 doi "https://doi.org/10.1029/91ja03020" @default.
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