Solitary Electromagnetic Pulses Detected with Super-Alfvénic Flows in Earth’s Geomagnetic Tail

dc.contributor.authorParks, G. K.
dc.contributor.authorLee, E.
dc.contributor.authorLin, N.
dc.contributor.authorMozer, F.
dc.contributor.authorWilber, M.
dc.contributor.authorDandouras, I.
dc.contributor.authorRème, H.
dc.contributor.authorLucek, E.
dc.contributor.authorFazakerley, A.
dc.contributor.authorGoldstein, Melvyn
dc.contributor.authorGurgiolo, C.
dc.contributor.authorCanu, P.
dc.contributor.authorCornilleau-Wehrlin, N.
dc.contributor.authorDécréau, P.
dc.date.accessioned2023-11-13T19:53:00Z
dc.date.available2023-11-13T19:53:00Z
dc.date.issued2007-06-27
dc.description.abstractSolitary nonlinear ( δB=B >> 1) electromagnetic pulses have been detected in Earth’s geomagnetic tail accompanying plasmas flowing at super-Alfvenic speeds. The pulses in the current sheet had durations of ∼5 s, were left-hand circularly polarized, and had phase speeds of approximately the Alfven speed in the plasma frame. These pulses were associated with a field-aligned current Jₗₗ and observed in low density (0:3 cm⁻³), high temperature (Te ∼ Ti ∼ 3 x 10⁷ K), and β ∼ 10 plasma that included electron and ion beams streaming along B. The wave activity was enhanced from below the ion cyclotron frequency to electron cyclotron and upper hybrid frequencies. The detailed properties suggest the pulses are nonlinearly steepened ion cyclotron or Alfven waves.en_US
dc.description.sponsorshipThe research at UC Berkeley is funded by a cluster data analysis grant, NASA Grant No. NNG04GF23G.en_US
dc.description.urihttps://journals.aps.org/prl/abstract/10.1103/PhysRevLett.98.265001en_US
dc.format.extent4 pagesen_US
dc.genrejournal articlesen_US
dc.identifierdoi:10.13016/m2sdlt-xsen
dc.identifier.citationParks, G. K., E. Lee, N. Lin, F. Mozer, M. Wilber, I. Dandouras, H. Rème, et al. “Solitary Electromagnetic Pulses Detected with Super-Alfv\’enic Flows in Earth’s Geomagnetic Tail.” Physical Review Letters 98, no. 26 (June 27, 2007): 265001. https://doi.org/10.1103/PhysRevLett.98.265001.en_US
dc.identifier.urihttps://doi.org/10.1103/PhysRevLett.98.265001
dc.identifier.urihttp://hdl.handle.net/11603/30744
dc.language.isoen_USen_US
dc.publisherAPSen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Goddard Planetary Heliophysics Institute (GPHI)
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.en_US
dc.rightsPublic Domain Mark 1.0*
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleSolitary Electromagnetic Pulses Detected with Super-Alfvénic Flows in Earth’s Geomagnetic Tailen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0002-5317-988Xen_US

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