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2022 Session 16. Heliospheric Turbulence II: Multiscale Nature of Turbulence from Inertial Scales to Dissipation Range Archives - SHINE

Nature and Scalings of Density Fluctuations of Compressible MHD Turbulence with Applications to the Solar Wind

Authors: Xiangrong Fu (New Mexico Consortium), Hui Li (Los Alamos National Laboratory), Zhaoming Gan (New Mexico Consortium), John Steinberg (Los Alamos National Laboratory) The solarView More

Guide field dependence of energy spectrum and energy transfer in reconnection

Authors: Michael Shay(University of Delaware), Tulasi N. Parashar (Victoria University of Wellington), William H. Matthaeus (University of Delaware) Classic picture of magnetic reconnection has shownView More

On the Estimation of Correlation Functions of Non-Contiguous Solar Wind Turbulence Signals

Authors: Mason Dorseth (Florida Institute of Technology), Jean C. Perez (Florida Institute of Technology), Sofiane Bourouaine (Johns Hopkins Applied Physics Laboratory), Juan Carlos Palacios CaicedoView More

Parametric Decay of Circularly Polarized Alfven Wave: One Dimensional and Multidimensional Simulations

Authors: Noshin Mashayekhizadeh(University of New Hampshire), Benjamin D G Chandran(University of New Hampshire), Kai Germaschewski(University of New Hampshire) In parametric decay, the presence of aView More

In-Situ Signature of Cyclotron Resonant Heating

Authors: Trevor A. Bowen (UC Berkeley), Ben Chandran (UNH), Jonathan Squire (Univ. Otago), Stuart D. Bale (UC Berkeley),Die Duan (Peking University), Kristopher G. Klein (U.View More

Laboratory Study of Alfvén Wave Parametric Instabilites

Authors: S. Dorfman (Space Science Institute), T. Carter (UCLA), S. Vincena (UCLA), F. Li (New Mexico Consortium), S. Fu (New Mexico Consortium), P. Pribyl (UCLA),View More

A Measure of Alfvenic Turbulence during PSP encounters 6, 7, and 8

Authors: Michael Terres (The University of Alabama in Huntsville), Gang Li (The University of Alabama in Huntsville) The solar wind is a superposition of variousView More

The Effects of Non-Equilibrium Velocity Distributions on Ion-Scale Waves in the Solar Wind

Authors: J. Walters (University of Arizona), K. G. Klein (University of Arizona), B. D. G. Chandran (University of New Hampshire), M. L. Stevens (Harvard SmithsonianView More

Effects of distribution structure on predictions of plasma behavior in marginally unstable plasma

Authors: E. Lichko (University of Arizona), K. Klein (University of Arizona) Due to low collisionality in space and astrophysical plasmas, distributions of ions and electronsView More

An extended and fragmented Alfvén zone in the Young Solar Wind

Authors: Rohit Chhiber (University of Delaware & NASA GSFC), William Matthaeus (University of Delaware), Arcadi Usmanov (University of Delaware & NASA GSFC), Riddhi Bandyopadhyay (PrincetonView More

Ion cyclotron waves in the solar wind and their indications of source ion distributions

Authors: H. Y. Wei (Dept. of Earth, Planetary and Space Sciences, University of California, Los Angeles, CA, USA), L. K. Jian (NASA Goddard Space FlightView More

HelioSwarm: Characterizing the Multi-Scale Nature of Space Plasma Turbulence

Authors: K.G. Klein, H. Spence, & the HelioSwarm Science and Engineering Teams Turbulence is multiscale disorder. It arises in a variety of astrophysical and heliosphericView More

Relative heating of protons and electrons in the young solar wind due to turbulent dissipation mediated by Landau damping

Authors: Niranjana Shankarappa (University of Arizona), Kristopher Klein (University of Arizona) The heating of protons and electrons as the result of the dissipation of turbulenceView More

Polarimeter to UNify the Corona and Heliosphere (PUNCH)

Authors: Don Kolinski (High Altitude Observatory, National Center for Atmospheric Research), Craig DeForest (Southwest Research Institute), Sarah Gibson (High Altitude Observatory, National Center for AtmosphericView More

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