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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 2.

Source alignment occurrences between PSP and SO. Panel (a): bulk solar wind speed; panel (b): Spacecraft radial distance; panel (c): coronal magnetic field expansion factor derived from the PFSS model; panel (d): Carrington latitude of the photospheric footpoints. The bulk speed in panel (a) is averaged over the injection time τinj (see Appendix A.1 for the details). Panels (a) and (b) show PSP and SO observations using horizontal crosses and dots, respectively. Mean trends are represented by running averages over 10 occurrences, shown with solid and dashed lines for PSP and SO, respectively, in panel (a). The corresponding PSP encounters for each alignment are indicated in panel (b) and separated by vertical dashed lines.

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