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On the Radial Evolution of the Solar Wind: The Source Alignment Method Applied to Parker Solar Probe and Solar Orbiter Observations

  • Authors: Jean-Baptiste Dakeyo, Tamar Ervin, Stuart Bale, Pascal Démoulin, Nikos Sioulas, Victor Réville, Mingzhe Liu, Alexis Rouillard, Milan Maksimovic, Davin Larson, Orlando Romeo, Philippe Louarn, Roberto Livi

Jean-Baptiste Dakeyo et al 2026 The Astrophysical Journal 1006 .

  • Provider: AAS Journals

Caption: Figure 5.

Correlation matrices of plasma parameters observed at PSP and SO within source alignments. Left panel: cross-correlation matrix for PSP alignment observations. Right panel: cross-correlation matrix for SO alignment observations. All quantities are averaged over τinj. Because the quantities span different orders of magnitude and are typically related by power laws, logarithmic values are used when computing correlations. As the diagonal elements represent autocorrelations, their coefficients are equal to unity by definition. Owing to the symmetry of the matrices, only the upper-right portions are displayed.

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