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Modification of the Power Spectral Density of Magnetic Field Fluctuations by Quasi-perpendicular Interplanetary Shocks

  • Authors: Byeongseon Park, Alexander Pitňa, Jana Šafránková, Zdeněk Němeček

Byeongseon Park et al 2025 The Astrophysical Journal Letters 986 .

  • Provider: AAS Journals

Caption: Figure 4.

Correlations between transition range spectral index ﹩{\alpha }_{{\rm{tr}}}﹩ and turbulence parameters estimated over 10 minute intervals. (a) ﹩{\alpha }_{{\rm{tr}}}﹩ vs. the absolute value of normalized cross helicity ∣σc∣, (b) ﹩{\alpha }_{{\rm{tr}}}﹩ vs. normalized fluctuation amplitude σB, and (c) ﹩{\alpha }_{{\rm{tr}}}﹩ vs. bulk speed ∣V∣. Dots and vertical bars indicate medians and their error; horizontal dashed lines show parameter medians and interquartiles. (d) Radial trends of ∣σc∣ and σB for FF shocks (upstream: black/green; downstream: red/blue). (e) Corresponding trend in ﹩{\alpha }_{{\rm{tr}}}﹩. Data are drawn from SolO, PSP, and Wind FF shock sets.

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