2 papers
astro-ph.SR2024
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…
astro-ph.SR2024
Solar wind data analysis aided by synthetic modeling: a better understanding of plasma-frame variations from temporal data
Norbert Magyar, Jaye Verniero, Adam Szabo +2
In-situ measurements of the solar wind, a turbulent and anisotropic plasma flow originating at the Sun, are mostly carried out by single spacecraft, resulting in one-dimensional ti…