M
Melvyn L. Goldstein
Researcher at University of Maryland, Baltimore County
Publications - 23
Citations - 1352
Melvyn L. Goldstein is an academic researcher from University of Maryland, Baltimore County. The author has contributed to research in topics: Solar wind & Magnetohydrodynamics. The author has an hindex of 13, co-authored 23 publications receiving 942 citations. Previous affiliations of Melvyn L. Goldstein include Durham University & Goddard Space Flight Center.
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Journal ArticleDOI
Highly structured slow solar wind emerging from an equatorial coronal hole
Stuart D. Bale,Samuel T. Badman,John W. Bonnell,Trevor A. Bowen,David Burgess,Anthony W. Case,Cynthia A Cattell,Benjamin D. G. Chandran,C. C. Chaston,Christopher H. K. Chen,James Drake,T. Dudok de Wit,Jonathan Eastwood,Robert E. Ergun,William M. Farrell,C. Fong,Keith Goetz,Melvyn L. Goldstein,Melvyn L. Goldstein,Katherine Goodrich,Peter Harvey,Timothy S. Horbury,Gregory G. Howes,Justin C. Kasper,Justin C. Kasper,Paul J. Kellogg,James A. Klimchuk,Kelly E. Korreck,Vladimir Krasnoselskikh,Säm Krucker,Säm Krucker,R. Laker,Davin Larson,Robert J. MacDowall,Milan Maksimovic,David M. Malaspina,J. C. Martínez-Oliveros,D. J. McComas,Nicole Meyer-Vernet,Michel Moncuquet,F. S. Mozer,Tai Phan,Marc Pulupa,N.-E. Raouafi,Chadi Salem,David Stansby,Michael L. Stevens,Adam Szabo,Marco Velli,T. Woolley,John R. Wygant +50 more
TL;DR: Measurements from the Parker Solar Probe show that slow solar wind near the Sun’s equator originates in coronal holes, and plasma-wave measurements suggest the existence of electron and ion velocity-space micro-instabilities that are associated with plasma heating and thermalization processes.
Journal ArticleDOI
Evaluation of magnetic helicity in homogeneous turbulence
TL;DR: In this article, a technique for the measurement of magnetic helicity from values of the two point magnetic field correlation matrix under the assumption of spatial homogeneity is presented, where knowledge of a single scalar function of space, derivable from the correlation matrix, suffices to determine the magnetic heliometry.
Journal ArticleDOI
Turbulence Analysis of the Jovian Upstream 'Wave' Phenomenon
TL;DR: In this article, an analysis of the magnetic field and plasma observations using spectral methods is presented, which is consistent with the hypothesis that these fluctuations are driven by streaming ions, possibly protons.
Journal ArticleDOI
The Solar Orbiter magnetometer
Timothy S. Horbury,Helen O'Brien,I. Carrasco Blazquez,M. Bendyk,Patrick Brown,R. Hudson,Vincent Evans,T. Oddy,Chris Carr,T. Beek,Emanuele Cupido,S. Bhattacharya,J.-A. Dominguez,L. Matthews,V. R. Myklebust,Barry J. Whiteside,Stuart D. Bale,Wolfgang Baumjohann,David Burgess,Vincenzo Carbone,Peter J. Cargill,Jonathan Eastwood,G. Erdös,Lyndsay Fletcher,R. J. Forsyth,Joe Giacalone,Karl-Heinz Glassmeier,Melvyn L. Goldstein,T. Hoeksema,Mike Lockwood,Werner Magnes,Milan Maksimovic,Eckart Marsch,William H. Matthaeus,Neil Murphy,Valery M. Nakariakov,Christopher J. Owen,Mathew J. Owens,Javier Rodriguez-Pacheco,Ingo Richter,Pete Riley,Christopher T. Russell,Steven J. Schwartz,Rami Vainio,Marco Velli,Susanne Vennerstrøm,Roger Walsh,Robert F. Wimmer-Schweingruber,Gary P. Zank,Daniel Müller,I. Zouganelis,Andrew Walsh +51 more
TL;DR: The magnetometer instrument on the Solar Orbiter mission is designed to measure the magnetic field local to the spacecraft continuously for the entire mission duration as discussed by the authors, and the overall instrument design, performance, data products, and operational strategy are described.