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Strong Prevalence of Hammerhead Velocity Distributions Close to the Heliospheric Current Sheet

  • Authors: Srijan Bharati Das, Jaye L. Verniero, Samuel T. Badman, Robert Alexander, Michael Terres, Federico Fraschetti, Kristoff W. Paulson, Fernando Carcaboso, Tatiana Niembro, Roberto Livi, Davin Larson, Ali Rahmati, Yeimy J. Rivera, Niranjana, Kristopher G. Klein, Michael L. Stevens

Srijan Bharati Das et al 2026 The Astrophysical Journal Letters 1001 .

  • Provider: AAS Journals

Caption: Figure 6.

The same as Figure 3, showing: (a) the PSP trajectory colored by r2BR(r) (red indicates positive polarity and blue indicates negative polarity); (b) the hammerhead occurrence fraction nham/ntotal proportional to the size of the lime green circles centered at each 1° bin along the PSP trajectory; and (c) the modeled HCS in solid black from E04–E13. The orange (blue) shaded regions indicate coronal holes formed by radially outgoing (incoming) open magnetic field lines.

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