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Abstract: On the Role of Elsasser Imbalance and Plasma β in Shaping the Statistical Properties of Sub-Ion Scale Turbulence and the Partitioning of Electron–Ion Heating in the Solar Wind (AGU25)

On the Role of Elsasser Imbalance and Plasma β in Shaping the Statistical Properties of Sub-Ion Scale Turbulence and the Partitioning of Electron–Ion Heating in the Solar Wind

Nikos Sioulas1, Trevor Bowen2, Alfred Mallet3, Benjamin D G Chandran4, Stuart D Bale2 and Jinsong Zhao5, (1)University of California Berkeley, Berkeley, CA, United States, (2)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (3)University of California Berkeley, Space Sciences Laboratory, Berkeley, United States, (4)University of New Hampshire, Durham, United States, (5)Purple Mountain Observatory, Chinese Academy of Sciences,, Nanjing, China