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The Impact of Alfvénic Shear Flow on Magnetic Reconnection and Turbulence

  • Authors: Tamar Ervin, Alfred Mallet, Stefan Eriksson, M. Swisdak, James Juno, Orlando M. Romeo, Tai Phan, Trevor A. Bowen, Roberto Livi, Phyllis L. Whittlesey, Davin E. Larson, Stuart D. Bale

Tamar Ervin et al 2025 The Astrophysical Journal Letters 992 .

  • Provider: AAS Journals

Caption: Figure 3.

Comparison of γtr/γ0tr (blue) and normalized flow shear (black) for (a) fast wind streams, (b) slow Alfvénic wind streams, and (c) slow wind streams. Wind is identified as fast, slow Alfvénic, or slow non-Alfvénic based on the categorization scheme of T. Ervin et al. (2024a).

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