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

Characterizing waves near the heliospheric current sheet with improved minimum variance analysis of PSP observations

Authors: Alexandre L. Brosius (PSU/NASA GSFC), Jaye L. Verniero (NASA GSFC), Adam Szabo (NASA GSFC) Parker Solar Probe is allowing us to witness magnetic reconnectionView 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

Sunward Strahl in Magnetic Field Reversals: Solar Connectivity and Magnetic Topology during Rapid Switchbacks in Parker Solar Probe Fast Electron Data

Authors: Phyllis Whittlesey (UCB/SSL), Justin Kasper (BWXT), Davin Larson(UCB/SSL), Michael Stevens (SAO), Anthony Case (SAO), Orlando Romeo(UCB/SSL), Jasper Halekas (U Iowa), Ali Rahmati (UCB/SSL) TheView 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

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

Phase Space Energization Analysis of the Corrugation Instability using the Field-Particle Correlation Technique

Authors: Collin Brown (University of Iowa), James Juno (Princeton Plasma Physics Laboratory), Greg Howes (University of Iowa), Colby Haggerty (University of Hawaii), Sage Constantinou (UniversityView More

Classification of Solar Wind Instabilities in the Inner Heliosphere

Authors: Mihailo M. Martinovic (University of Arizona), Kristopher G. Klein (University of Arizona), Tereza Durovcova (Charles University, Prague), Benjamin L. Alterman (Southwest Research Institute) InstabilitiesView 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

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