N
Neil Murphy
Researcher at Jet Propulsion Laboratory
Publications - 86
Citations - 1587
Neil Murphy is an academic researcher from Jet Propulsion Laboratory. The author has contributed to research in topics: Solar wind & Heliosphere. The author has an hindex of 19, co-authored 79 publications receiving 1321 citations. Previous affiliations of Neil Murphy include Nanyang Technological University & California Institute of Technology.
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Journal ArticleDOI
The heliospheric plasma sheet
TL;DR: In this article, high-resolution magnetic field and plasma data gathered by ISEE 3/ICE during several sector boundary crossings are used to investigate the narrow heliospheric current sheet (approximately equal 3 x 10 (exp 3) km to 10(exp 4) km) together with the heliosphere plasma sheet in which it is embedded.
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Magnetic field observations during the ulysses flyby of jupiter.
A. Balogh,Michele K. Dougherty,R. J. Forsyth,David J. Southwood,Edward J. Smith,Bruce T. Tsurutani,Neil Murphy,M. E. Burton +7 more
TL;DR: The Jovian flyby of the Ulysses spacecraft presented the opportunity to confirm and complement the findings of the four previous missions that investigated the structure and dynamics of theJovian magnetosphere and magnetic field, as well as to explore for the first time the high-latitude dusk side of the magnetosphere
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Understanding coronal heating and solar wind acceleration: Case for in situ near‐Sun measurements
David J. McComas,Marco Velli,Marco Velli,W. S. Lewis,Loren W. Acton,M. Balat-Pichelin,Volker Bothmer,R. B. Dirling,W. C. Feldman,George Gloeckler,S. R. Habbal,Donald M. Hassler,I. Mann,William H. Matthaeus,Ralph L. McNutt,R. A. Mewaldt,Neil Murphy,Leon Ofman,Edward C. Sittler,Charles W. Smith,Thomas H. Zurbuchen +20 more
TL;DR: In situ observations near the Sun, from a few solar radii (R_S) out to ∼20 R_S, where the internal, magnetic, and turbulent energy in the coronal plasma is channeled into the bulk energy of the supersonic solar wind has been a top priority of the solar and space physics community as mentioned in this paper.
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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.
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Energetic particle signatures at Ganymede: Implications for Ganymede's magnetic field
D. J. Williams,Barry Mauk,R. W. McEntire,Edmond C. Roelof,Thomas P. Armstrong,B. Wilken,Juan G. Roederer,Stamatios M. Krimigis,Theodore A. Fritz,Louis J. Lanzerotti,Neil Murphy +10 more
TL;DR: The second encounter of the Galileo satellite with the Galilean moon Ganymede provided energetic particle measurements showing effects due to the presence of that moon as mentioned in this paper, where the Energetic Particles Detector (EPD) views along the magnetic field line.