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Global observations of magnetospheric high‐m poloidal waves during the 22 June 2015 magnetic storm

dc.contributor.authorLe, G.
dc.contributor.authorChi, P. J.
dc.contributor.authorStrangeway, R. J.
dc.contributor.authorRussell, C. T.
dc.contributor.authorSlavin, J. A.
dc.contributor.authorTakahashi, K.
dc.contributor.authorSinger, H. J.
dc.contributor.authorAnderson, B. J.
dc.contributor.authorBromund, K.
dc.contributor.authorFischer, D.
dc.contributor.authorKepko, E. L.
dc.contributor.authorMagnes, W.
dc.contributor.authorNakamura, R.
dc.contributor.authorPlaschke, F.
dc.contributor.authorTorbert, R. B.
dc.date.accessioned2017-06-16T20:15:53Z
dc.date.available2018-06-01T13:51:00Zen
dc.date.issued2017-04-28
dc.identifier.citationLe, G.; Chi, P. J.; Strangeway, R. J.; Russell, C. T.; Slavin, J. A.; Takahashi, K.; Singer, H. J.; Anderson, B. J.; Bromund, K.; Fischer, D.; Kepko, E. L.; Magnes, W.; Nakamura, R.; Plaschke, F.; Torbert, R. B. (2017). "Global observations of magnetospheric high‐m poloidal waves during the 22 June 2015 magnetic storm." Geophysical Research Letters 44(8): 3456-3464.
dc.identifier.issn0094-8276
dc.identifier.issn1944-8007
dc.identifier.urihttps://hdl.handle.net/2027.42/137558
dc.description.abstractWe report global observations of high‐m poloidal waves during the recovery phase of the 22 June 2015 magnetic storm from a constellation of widely spaced satellites of five missions including Magnetospheric Multiscale (MMS), Van Allen Probes, Time History of Events and Macroscale Interactions during Substorm (THEMIS), Cluster, and Geostationary Operational Environmental Satellites (GOES). The combined observations demonstrate the global spatial extent of storm time poloidal waves. MMS observations confirm high azimuthal wave numbers (m ~ 100). Mode identification indicates the waves are associated with the second harmonic of field line resonances. The wave frequencies exhibit a decreasing trend as L increases, distinguishing them from the single‐frequency global poloidal modes normally observed during quiet times. Detailed examination of the instantaneous frequency reveals discrete spatial structures with step‐like frequency changes along L. Each discrete L shell has a steady wave frequency and spans about 1 RE, suggesting that there exist a discrete number of drift‐bounce resonance regions across L shells during storm times.Key PointsObserved long‐lasting high‐m poloidal waves associated with second harmonics of field line resonances during a major magnetic stormDemonstrated global spatial extent of storm time poloidal FLR region using observations from a constellation of widely spaced satellitesRevealed discrete spatial structures of resonant L shells with step‐like frequency changes
dc.publisherWiley Periodicals, Inc.
dc.publisherAGU
dc.subject.otherULF waves
dc.subject.othermagnetic storm
dc.subject.otherfield line resonances
dc.subject.otherhigh‐m poloidal waves
dc.subject.othermagnetospheric multiscale mission
dc.titleGlobal observations of magnetospheric high‐m poloidal waves during the 22 June 2015 magnetic storm
dc.typeArticleen_US
dc.rights.robotsIndexNoFollow
dc.subject.hlbsecondlevelGeological Sciences
dc.subject.hlbtoplevelScience
dc.description.peerreviewedPeer Reviewed
dc.description.bitstreamurlhttps://deepblue.lib.umich.edu/bitstream/2027.42/137558/1/grl55775_am.pdf
dc.description.bitstreamurlhttps://deepblue.lib.umich.edu/bitstream/2027.42/137558/2/grl55775.pdf
dc.identifier.doi10.1002/2017GL073048
dc.identifier.sourceGeophysical Research Letters
dc.identifier.citedreferenceSinger, H. J., W. J. Hughes, and C. T. Russell ( 1982 ), Standing hydromagnetic waves observed by ISEE 1 and 2: Radial extent and harmonic, J. Geophys. Res., 87 ( A5 ), 3519 – 3529, doi: 10.1029/JA087iA05p03519.
dc.identifier.citedreferenceChen, L., and A. Hasegawa ( 1988 ), On magnetospheric hydromagnetic waves excited by energetic ring‐current particles, J. Geophys. Res., 93 ( A8 ), 8763 – 8767, doi: 10.1029/JA093iA08p08763.
dc.identifier.citedreferenceChen, L., and A. Hasegawa ( 1991 ), Kinetic theory of geomagnetic pulsations: 1. Internal excitations by energetic particles, J. Geophys. Res., 96 ( A2 ), 1503 – 1512, doi: 10.1029/90JA02346.
dc.identifier.citedreferenceCheng, C. Z., T. C. Chang, C. A. Lin, and W. H. Tsai ( 1993 ), Magnetohydrodynamic theory of field line resonances in the magnetosphere, J. Geophys. Res., 98 ( A7 ), 11339 – 11347, doi: 10.1029/93JA00505.
dc.identifier.citedreferenceChi, P. J., and G. Le ( 2015 ), Observations of magnetospheric high‐ m poloidal waves by ST‐5 satellites in low Earth orbit during geomagnetically quiet times, J. Geophys. Res. Space Physics, 120, 4776 – 4783, doi: 10.1002/2015JA021145.
dc.identifier.citedreferenceChi, P. J., and C. T. Russell ( 2008 ), Use of the Wigner‐Ville distribution in interpreting and identifying ULF waves in triaxial magnetic records, J. Geophys. Res., 113, A01218, doi: 10.1029/2007JA012469.
dc.identifier.citedreferenceDai, L., et al. ( 2015 ), Storm time occurrence and spatial distribution of Pc4 poloidal ULF waves in the inner magnetosphere: A Van Allen Probes statistical study, J. Geophys. Res. Space Physics, 120, 4748 – 4762, doi: 10.1002/2015JA021134.
dc.identifier.citedreferenceDenton, R. E., and G. Vetoulis ( 1998 ), Global poloidal mode, J. Geophys. Res., 103 ( A4 ), 6729 – 6739, doi: 10.1029/97JA03594.
dc.identifier.citedreferenceDenton, R. E., M. R. Lessard, and L. M. Kistler ( 2003 ), Radial localization of magnetospheric guided poloidal Pc 4–5 waves, J. Geophys. Res., 108 ( A3 ), 1105, doi: 10.1029/2002JA009679.
dc.identifier.citedreferenceEngebretson, M. J., D. L. Murr, K. N. Erickson, R. J. Strangeway, D. M. Klumpar, S. A. Fuselier, L. J. Zanetti, and T. A. Potemra ( 1992 ), The spatial extent of radial magnetic pulsation events observed in the dayside near synchronous orbit, J. Geophys. Res., 97 ( A9 ), 13741 – 13758, doi: 10.1029/92JA00992.
dc.identifier.citedreferenceEriksson, P. T. I., L. G. Blomberg, A. D. M. Walker, and K.‐H. Glassmeier ( 2005 ), Poloidal ULF oscillations in the dayside magnetosphere: A Cluster study, Ann. Geophys., 23, 2679 – 2686, doi: 10.5194/angeo‐23‐2679‐2005.
dc.identifier.citedreferenceHasegawa, A., and L. Chen ( 1989 ), Theory of the drift mirror instability, in Plasma Waves and Instabilities at Comets and in Magnetospheres, edited by B. T. Tsurutani and H. Oya, pp. 173 – 177, AGU, Washington, D. C., doi: 10.1029/GM053p0173.
dc.identifier.citedreferenceHudson, M., R. Denton, M. Lessard, E. Miftakhova, and R. Anderson ( 2004 ), A study of Pc‐5 ULF oscillations, Ann. Geophys., 22, 289 – 302.
dc.identifier.citedreferenceHughes, W. J., and D. J. Southwood ( 1976 ), The screening of micropulsation signals by the atmosphere and ionosphere, J. Geophys. Res., 81 ( 19 ), 3234 – 3240.
dc.identifier.citedreferenceHughes, W. J., R. L. McPherron, J. N. Barfield, and B. H. Mauk ( 1979 ), A compressional Pc4 pulsation observed by three satellites in geostationary orbit near local midnight, Planet. Space Sci., 27, 821 – 840.
dc.identifier.citedreferenceKokubun, S., K. N. Erickson, T. A. Fritz, and R. L. McPherron ( 1989 ), Local time asymmetry of Pc 4–5 pulsations and associated particle modulations at synchronous orbit, J. Geophys. Res., 94 ( A6 ), 6607 – 6625, doi: 10.1029/JA094iA06p06607.
dc.identifier.citedreferenceKorotova, G. I., D. G. Sibeck, M. J. Engebretson, J. R. Wygant, S. Thaller, H. E. Spence, C. A. Kletzing, V. Angelopoulos, and R. J. Redmon ( 2016 ), Multipoint spacecraft observations of long‐lasting poloidal Pc4 pulsations in the dayside magnetosphere on May 1–2, 2014, Ann. Geophys., 34, 985 – 998, doi: 10.5194/angeo‐34‐985‐2016.
dc.identifier.citedreferenceLe, G., P. J. Chi, R. J. Strangeway, and J. A. Slavin ( 2011 ), Observations of a unique type of ULF wave by low‐altitude Space Technology 5 satellites, J. Geophys. Res., 116, A08203, doi: 10.1029/2011JA016574.
dc.identifier.citedreferenceLiu, W., T. E. Sarris, X. Li, S. R. Elkington, R. Ergun, V. Angelopoulos, J. Bonnell, and K. H. Glassmeier ( 2009 ), Electric and magnetic field observations of Pc4 and Pc5 pulsations in the inner magnetosphere: A statistical study, J. Geophys. Res., 114, A12206, doi: 10.1029/2009JA014243.
dc.identifier.citedreferenceLiu, Y. D., H. Hu, R. Wang, Z. Yang, B. Zhu, Y. A. Liu, J. G. Luhmann, and J. D. Richardson ( 2015 ), Plasma and magnetic field characteristics of solar coronal mass ejections in relation to geomagnetic storm intensity and variability, Astrophys. J. Lett., 809 ( 2 ), doi: 10.1088/2041‐8205/809/2/L34.
dc.identifier.citedreferenceNosé, M., et al. ( 2015 ), Formation of the oxygen torus in the inner magnetosphere: Van Allen Probes observations, J. Geophys. Res. Space Physics, 120, 1182 – 1196, doi: 10.1002/2014JA020593.
dc.identifier.citedreferenceSchäfer, S., K. H. Glassmeier, P. T. I. Eriksson, V. Pierrard, K. H. Fornaçon, and L. G. Blomberg ( 2007 ), Spatial and temporal characteristics of poloidal waves in the terrestrial plasmasphere: A CLUSTER case study, Ann. Geophys., 25, 1011 – 1024, doi: 10.5194/angeo‐25‐1011‐2007.
dc.identifier.citedreferenceSugiura, M., and C. R. Wilson ( 1964 ), Oscillation of the geomagnetic field lines and associated magnetic perturbations at conjugate points, J. Geophys. Res., 69 ( 7 ), 1211 – 1216, doi: 10.1029/JZ069i007p01211.
dc.identifier.citedreferenceSouthwood, D. J. ( 1974 ), Some features of field line resonances in the magnetosphere, Planet. Space Sci., 22, 483 – 491.
dc.identifier.citedreferenceSouthwood, D. J., J. W. Dungey, and R. J. Etherington ( 1969 ), Bounce resonant interaction between pulsations and trapped particles, Planet. Space Sci., 17 ( 3 ), 349 – 361, doi: 10.1016/0032‐0633(69)90068‐3.
dc.identifier.citedreferenceTakahashi, K., P. R. Higbie, and D. N. Baker ( 1985a ), Azimuthal propagation and frequency characteristic of compressional Pc 5 waves observed at geostationary orbit, J. Geophys. Res., 90 ( A2 ), 1473 – 1485, doi: 10.1029/JA090iA02p01473.
dc.identifier.citedreferenceTakahashi, K., C. T. Russell, and R. R. Anderson ( 1985b ), ISEE 1 and 2 observation of the spatial structure of a compressional Pc 5 wave, Geophys. Res. Lett., 12, 613, doi: 10.1029/GL012i009p00613.
dc.identifier.citedreferenceTakahashi, K., J. F. Fennell, E. Amata, and P. R. Higbie ( 1987 ), Field‐aligned structure of the storm time Pc 5 wave of November 14–15, 1979, J. Geophys. Res., 92 ( A6 ), 5857 – 5864, doi: 10.1029/JA092iA06p05857.
dc.identifier.citedreferenceTakahashi, K., K.‐H. Glassmeier, V. Angelopoulos, J. Bonnell, Y. Nishimura, H. J. Singer, and C. T. Russell ( 2011 ), Multisatellite observations of a giant pulsation event, J. Geophys. Res., 116, A11223, doi: 10.1029/2011JA016955.
dc.identifier.citedreferenceTakahashi, K., M. D. Hartinger, V. Angelopoulos, K.‐H. Glassmeier, and H. J. Singer ( 2013 ), Multispacecraft observations of fundamental poloidal waves without ground magnetic signatures, J. Geophys. Res. Space Physics, 118, 4319 – 4334, doi: 10.1002/jgra.50405.
dc.identifier.citedreferenceVetoulis, G., and L. Chen ( 1994 ), Global structures of Alfvén‐ballooning modes in magnetospheric plasmas, Geophys. Res. Lett., 21, 2091 – 2094, doi: 10.1029/94GL01703.
dc.identifier.citedreferenceVetoulis, G., and L. Chen ( 1996 ), Kinetic theory of geomagnetic pulsations: 3. Global analysis of drift Alfvén‐ballooning modes, J. Geophys. Res., 101 ( A7 ), 15441 – 15456, doi: 10.1029/96JA00494.
dc.identifier.citedreferenceZong, Q.‐G., X.‐Z. Zhou, Y. F. Wang, X. Li, P. Song, D. N. Baker, T. A. Fritz, P. W. Daly, M. Dunlop, and A. Pedersen ( 2009 ), Energetic electron response to ULF waves induced by interplanetary shocks in the outer radiation belt, J. Geophys. Res., 114, A10204, doi: 10.1029/2009JA014393.
dc.identifier.citedreferenceZhu, X., and M. G. Kivelson ( 1991 ), Compressional ULF waves in the outer magnetosphere: 1. Statistical study, J. Geophys. Res., 96 ( A11 ), 19451 – 19467, doi: 10.1029/91JA01860.
dc.identifier.citedreferenceAnderson, B. J., M. J. Engebretson, S. P. Rounds, L. J. Zanetti, and T. A. Potemra ( 1990 ), A statistical study of Pc 3–5 pulsations observed by the AMPTE/CCE Magnetic Fields Experiment: 1. Occurrence distributions, J. Geophys. Res., 95 ( A7 ), 10495 – 10523, doi: 10.1029/JA095iA07p10495.
dc.identifier.citedreferenceChen, L., and A. Hasegawa ( 1974 ), A theory of long‐period magnetic pulsations: 1. Steady state excitation of field line resonance, J. Geophys. Res., 79 ( 7 ), 1024 – 1032.
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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