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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 2.

Coincidence (COIN) rate spectra of SWAPI (J. S. Rankin et al. 2025) colored according to time in UTC (here each profile reflects 10 minute averages) together with the IMF recorded by MAG downsampled at 1 minute cadence. In the lower three panels, proton SW speed, density, and temperature are also shown at a 1 minute cadence. Steady SW can be identified during this period.

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