Figure 3 from Magnetic Reconnection as a Driver for a Sub-ion-scale Cascade in Plasma Turbulence

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Magnetic Reconnection as a Driver for a Sub-ion-scale Cascade in Plasma Turbulence

Authors: Luca Franci, Silvio Sergio Cerri, Francesco Califano, Simone Landi, Emanuele Papini, Andrea Verdini, Lorenzo Matteini, Frank Jenko, and Petr Hellinger

2017 The Astrophysical Journal Letters 850 L16.

Provider: AAS Journals

Caption: Figure 3.

(a) Power spectra of the parallel (top) and total (bottom) magnetic fluctuations for the HPIC run before (red) and after (orange) the first magnetic reconnection events occur, at an intermediate time (green) and when the quasi-steady state is reached (light blue). Characteristic power laws are drawn as a reference. (b) Same as in panel (a), but for the HVM run.

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