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Identifying Compressive Fluctuations In Inertial Range Solar Wind

Identifying Compressive Fluctuations In Inertial Range Solar Wind. K.G. Klein 1 , G.G. Howes 1 , S.D. Bale 2 , C.H.K. Chen 2 , C.S. Salem 2 , J.M. TenBarge 1. 1 University of Iowa 2 University of California, Berkeley. SHINE session: The Dissipation of Solar Wind Turbulence.

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Identifying Compressive Fluctuations In Inertial Range Solar Wind

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  1. Identifying Compressive Fluctuations In Inertial Range Solar Wind K.G. Klein1, G.G. Howes1, S.D. Bale2, C.H.K. Chen2, C.S. Salem2,J.M. TenBarge1 1University of Iowa 2University of California, Berkeley SHINE session: The Dissipation of Solar Wind Turbulence • C(δn, δB||) from ~1.2x105 WIND data intervals is ~-1 • Correlation implies that a preponderance of the compressive energy is due to slow waves • Lack of fast waves may have implications for in dissipation range Correlation of density and parallel magnetic fluctuations: Points from WIND data, Lines from synthetic data model.

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