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This page is a summary of: PHYSICAL INTERPRETATION OF THE ANGLE-DEPENDENT MAGNETIC HELICITY SPECTRUM IN THE SOLAR WIND: THE NATURE OF TURBULENT FLUCTUATIONS NEAR THE PROTON GYRORADIUS SCALE, The Astrophysical Journal, April 2014, Institute of Physics Publishing,
DOI: 10.1088/0004-637x/785/2/138.
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