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Recent Parker Solar Probe (PSP) observations of inner heliospheric plasma have shown an abundant presence of Alfv\ enic polarity reversal of the magnetic field, known as switchbacks. While their origin is still debated, their role in driving the solar wind turbulence has been suggested through analysis of the spectral properties of magnetic fluctuations. Here, we provide a complementary assessment of their role in the turbulent cascade. The validation of the third-order linear scaling of velocity and magnetic fluctuation ...
Published by: \apjl Published on: nov
YEAR: 2021   DOI: 10.3847/2041-8213/ac36d1
Published by: \apj Published on: 01/2017
YEAR: 2017   DOI: 10.3847/1538-4357/834/2/166