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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 1.

Schematic summary of our hammerhead detection algorithm used in hampy. All velocity phase-space plots are presented on an E − θ plane. The Vx − Vz coordinates are calculated by using ϕ ∼ 163﹩\mathop{.}\limits^{\unicode{x000b0}}﹩125. (a) ϕ-collapsed f(vxvz) in the SPAN-I instrument frame before preprocessing. (b) f(vxvz) after removing spurious count bins that do not form a contiguous distribution in the 2D (vxvz) space. (c) The same as panel (b) but plotted using contour levels in a cell-centered convention. The black lines represent slices along different instrument elevation angles. The red lines at θ ∼ −37° and 22° correspond to the elevations for the detected necks for the shown hammerhead distribution. The red grids in panels (e) and (f) show the detected necks using the corresponding 1D convolution profiles shown in panels (d1) and (d2). All VDF values are presented in log base 10.

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