Solar wind turbulence near Mercury shows stable -3/2 inertial-range spectra with no radial evolution but shallower kinetic-range spectra and evolving ion-scale breaks with increasing heliocentric distance.
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Properties and Radial Evolution of Solar Wind Turbulence Near Mercury's Orbit
Solar wind turbulence near Mercury shows stable -3/2 inertial-range spectra with no radial evolution but shallower kinetic-range spectra and evolving ion-scale breaks with increasing heliocentric distance.