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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 .

Caption: Figure 1.

The magnitude B of the IMF (black line) together with its radial B_R (blue line), transverse B_T (green line), and normal B_N (red line) components.