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William H. Matthaeus
Researcher at University of Delaware
Publications - 546
Citations - 34936
William H. Matthaeus is an academic researcher from University of Delaware. The author has contributed to research in topics: Solar wind & Magnetohydrodynamics. The author has an hindex of 93, co-authored 515 publications receiving 31310 citations. Previous affiliations of William H. Matthaeus include University of Calabria & University of California, Riverside.
Papers
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HelioSwarm: A Multipoint, Multiscale Mission to Characterize Turbulence
Kristopher Klein,Harlan E. Spence,Olga Alexandrova,Matthew R. Argall,Lev Arzamasskiy,Jay A. Bookbinder,Theodore Broeren,Damiano Caprioli,Anthony W. Case,Benjamin D. G. Chandran,Li-Jen Chen,I. Dors,Jonathan Eastwood,Colin Forsyth,Antoinette B. Galvin,Vincent Génot,Jasper Halekas,Michael Hesse,B. P. Hine,Timothy S. Horbury,Lan Jian,Justin C. Kasper,Matthieu Kretzschmar,Matthew W. Kunz,Benoit Lavraud,O. Le Contel,Alfred Mallet,Bennett A. Maruca,William H. Matthaeus,J. T. Niehof,Christopher J. Owen,Alessandro Retinò,Christopher Reynolds,Owen Roberts,Alexander Schekochihin,Ruth M. Skoug,Charles D. Smith,Sonya S. Smith,John T. Steinberg,Michael L. Stevens,Adam Szabo,Jason TenBarge,Roy B. Torbert,Bernard J. Vasquez,Daniel Verscharen,Phyllis Whittlesey,B. Wickizer,Gary P. Zank,Ellen G. Zweibel +48 more
TL;DR: HelioSwarm (HS) is a NASA Medium-Class Explorer mission of the Heliophysics Division designed to explore the dynamic three-dimensional mechanisms controlling the physics of plasma turbulence, a ubiquitous process occurring in the heliosphere and in plasmas throughout the universe as mentioned in this paper .
Proceedings ArticleDOI
Considerations limiting cyclotron-resonant damping of cascading interplanetary turbulence and why the ‘slab’ approximation fails
TL;DR: In this paper, an active spectral cascade into the dissipation range is balanced by a combination of resonant and nonresonant kinetic dissipation mechanisms, and the ratio of the two methods of dissipation is of order unity.
Proceedings ArticleDOI
Solar Wind Turbulent Heating by Interstellar Pickup Protons: 2‐Component Model
TL;DR: In this paper, a 2-component phenomenology was applied to the turbulent heating of the core solar wind protons as seen at the Voyager 2 spacecraft to improve the model predictions of core temperature and correlation scale.
Posted Content
Suprathermal Ion Energy spectra and Anisotropies near the Heliospheric Current Sheet crossing observed by the Parker Solar Probe during Encounter 7.
M. I. Desai,Donald G. Mitchell,D. J. McComas,James Drake,Tai Phan,J. R. Szalay,Edmond C. Roelof,Joe Giacalone,Matthew E. Hill,E. R. Christian,Nathan A. Schwadron,Ralph L. McNutt,M. E. Wiedenbeck,C. Joyce,C. M. S. Cohen,Andrew Davis,Stamatios M. Krimigis,R. A. Leske,William H. Matthaeus,Olga Malandraki,R. A. Mewaldt,A. W. Labrador,E. C. Stone,Stuart D. Bale,J. L. Verniero,Ali Rahmati,P. L. Whittlesey,Roberto Livi,Davin Larson,Marc Pulupa,Robert J. MacDowall,J. T. Niehof,Justin C. Kasper,Timothy S. Horbury +33 more
TL;DR: In this paper, the authors present observations of >10-100 keV/nucleon suprathermal (ST) H, He, O, and Fe ions associated with crossings of the heliospheric current sheet (HCS) at radial distances <0.1 au from the Sun.