Non‐self‐similar scaling of plasma sheet and solar wind probability distribution functions of magnetic field fluctuations
J. M. Weygand(Planetary Science Institute), M. L. Goldstein(Space Science Institute), L. M. Kistler(University of New Hampshire at Manchester), H. Schwarzl(Planetary Science Institute), R. J. Walker(Planetary Science Institute), M. G. Kivelson(Planetary Science Institute), A. Balogh(Imperial College London), K. K. Khurana(University of California, Los Angeles)
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