32 citations · 114 across the 6 of their papers we have counts for
6 papers
Two Types of Range in Solar Wind Turbulence
Zesen Huang, Marco Velli, B. D. G. Chandran +4
The noise is a ubiquitous phenomenon in natural systems. Since the advent of space exploration, the range has been consistently observed in \textit{in situ} solar wind…
Preferential Proton over Electron heating from coherent structures during the first perihelion of Parker Solar Probe
Nikos Sioulas, Chen Shi, Zesen Huang +1
The solar wind undergoes significant heating as it propagates away from the Sun; the exact mechanisms responsible for this heating remain unclear. Using data from the first perihel…
Magnetic field intermittency in the solar wind: PSP and SolO observations ranging from the Alfven region out to 1 AU
Nikos Sioulas, Zesen Huang, Marco Velli +17
and data are utilized to investigate magnetic field intermittency in the solar wind (SW). Small-scale intermittency is observed to radially strengthen…
Propagation of Alfvén waves in the expanding solar wind with the fast-slow stream interaction
Chen Shi, Marco Velli, Anna Tenerani +2
We carry out two-dimensional magnetohydrodynamic (MHD) simulations of an ensemble of Alfvénic fluctuations propagating in a structured, expanding solar wind including the presence…
Fast Recursive Reconnection and the Hall effect: Hall-MHD Simulations
Chen Shi, Anna Tenerani, Marco Velli +1
Magnetohydrodynamic (MHD) theory and simulations have shown that reconnection is triggered via a fast "ideal" tearing instability in current sheets whose inverse aspect ratio decre…
Marginal Stability of Sweet-Parker Type Current Sheets at Low Lundquist Numbers
Chen Shi, Marco Velli, Anna Tenerani
Magnetohydrodynamic simulations have shown that a non-unique critical Lundquist number exists, hovering around , above which threshold Sweet-Parker type statio…