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The Incompressible Magnetohydrodynamic Energy Cascade Rate Upstream of Mars: Effects of the Total Energy and the Cross-Helicity on Solar Wind Turbulence
Norberto Romanelli, Nahuel Andres, Gina DiBraccio +5
Solar wind turbulence is a dynamical phenomenon that evolves with heliocentric distance. Orbiting Mars since September 2014, Mars Atmosphere and Volatile EvolutioN (MAVEN) offers a…
Resonance of low-frequency electromagnetic and ion-sound modes in the solar wind
I. Y. Vasko, F. S. Mozer, T. Bowen +6
Parker Solar Probe measurements have recently shown that coherent fast magnetosonic and Alfvén ion-cyclotron waves are abundant in the solar wind and can be accompanied by higher-f…
On the Heating of the Slow Solar-Wind by Imbalanced Alfvén-Wave Turbulence from 0.06 au to 1 au: Parker Solar Probe and Solar Orbiter observations
Sofiane Bourouaine, Jean C. Perez, Benjamin D. G. Chandran +3
In this work we analyze plasma and magnetic field data provided by the Parker Solar Probe (\emph{PSP}) and Solar Orbiter (\emph{SO}) missions to investigate the radial evolution of…
Alfvén Waves at Mars
Norberto Romanelli, Christopher M. Fowler, Gina A. DiBraccio +2
The solar wind upstream of Mars's bow shock can be described in terms of Alfvénic turbulence, with an incompressible energy cascade rate of J m s at magnet…
Intermittent Electron-Only Reconnection at Lunar Mini-Magnetospheres
Adam Stanier, Li-Jen Chen, Ari Le +2
Lunar crustal magnetic anomalies (LCMA) are sub-ion-gyroradius structures that have been shown to stand off the solar wind (SW) plasma from the Moon's surface, forming shock-like d…
A Virtual Solar Wind Monitor at Mars with Uncertainty Quantification using Gaussian Processes
A. R. Azari, E. Abrahams, F. Sapienza +9
Single spacecraft missions do not measure the pristine solar wind continuously because of the spacecrafts' orbital trajectory. The infrequent spatiotemporal cadence of measurement…