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Similarity of Fluctuations in Correlated Systems: The Case of the Magnetic Field Measured at 1 au by IMAP during Steady Solar Wind

  • Authors: N. V. Sarlis, G. Livadiotis, D. J. McComas, N. A. Schwadron, M. Gkioulidou, M. E. Cuesta, J. S. Rankin, H. A. Farooki, S. Kasapis, L. Y. Khoo, M. M. Shen, B. L. Shrestha

N. V. Sarlis et al 2027 The Astrophysical Journal Supplement Series 288 .

  • Provider: AAS Journals

Caption: Figure 4.

(a) The scaled distribution of μW(κ1) for W = 600, 450, 300, and 150 for BR, BT, and BN for τc = 12 s. The continuous purple line corresponds to the scaled distribution of the magnetization of a 2D Ising model of linear dimension L = 50 below its critical temperature Tc with inverse temperature parameter K = 0.4677 (Kc = 0.4407, see K. Huang 1987) while the so-called (B. P. van Milligen et al. 2005) BHP function (see Equation (6)) can be also visualized in green. (b) The same as in (a) but for BR only with additional values of W and τc. (c), (d) The same as (b) but for BT, and BN, respectively.

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