Solar wind turbulence near Mercury's orbit shows stable inertial-range spectra but radially evolving kinetic-range spectra, with ion-scale breaks tied to local plasma conditions rather than proton cyclotron frequency.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
physics.space-ph 1years
2026 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Properties and Radial Evolution of Solar Wind Turbulence Near Mercury's Orbit
Solar wind turbulence near Mercury's orbit shows stable inertial-range spectra but radially evolving kinetic-range spectra, with ion-scale breaks tied to local plasma conditions rather than proton cyclotron frequency.