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• W2076386844 abstract "We present correlated particle and magnetic field measurements by the ISEE 3 spacecraft for the loop structure behind the interplanetary traveling shock event of November 12, 1978. Following the passage of the turbulent shock region, we observe strong bidirectional streaming of low‐energy protons for approximately 6 hours, corresponding to a loop thickness of about 0.07 AU. This region is also characterized by a low relative variance of the magnetic field, a depressed proton intensity, and a reduction in the magnetic power spectral density. Using quasi‐linear theory applied to a slab model, we derive a value of 3 AU for the mean free path during the passage of the closed loop. We infer from this observation that the proton régime associated with the loop structure is experiencing scatter‐free transport and that either the length of the loop is approximately 3 AU between the sun and the earth or else the protons are being reflected at both ends of a smaller loop." @default.
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• W2076386844 date "1987-01-01" @default.
• W2076386844 modified "2023-10-14" @default.
• W2076386844 title "Properties of a large-scale interplanetary loop structure as deduced from low-energy proton anisotropy and magnetic field measurements" @default.
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• W2076386844 doi "https://doi.org/10.1029/ja092ia01p00006" @default.
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