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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 3.

How a time series of BR (blue) in conventional (clock) time can be visualized in natural time (right panel). The left panel shows 2 Hz IMF components (colored circles) and magnitude (black line) during the period 04:00:00 to 04:10:00 UTC on 2025 December 1, together with their averaged values (continuous lines of darker color) with cadence τc = 4 s. The latter measurements are used for the estimation of the distribution of pk of NTA which is shown in the right panel. Here, N = 150 corresponding to 10 minutes with a cadence of 4 s.

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