Magnetospheric “magic” frequencies as magnetopause surface eigenmodes
dc.contributor.author | Archer, M. O. | en_US |
dc.contributor.author | Hartinger, M. D. | en_US |
dc.contributor.author | Horbury, T. S. | en_US |
dc.date.accessioned | 2013-11-01T19:01:07Z | |
dc.date.available | 2014-11-03T16:20:38Z | en_US |
dc.date.issued | 2013-10-16 | en_US |
dc.identifier.citation | Archer, M. O.; Hartinger, M. D.; Horbury, T. S. (2013). "Magnetospheric “magic” frequencies as magnetopause surface eigenmodes." Geophysical Research Letters 40(19): 5003-5008. <http://hdl.handle.net/2027.42/100327> | en_US |
dc.identifier.issn | 0094-8276 | en_US |
dc.identifier.issn | 1944-8007 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/100327 | |
dc.publisher | Springer‐Verlag Berlin | en_US |
dc.publisher | Wiley Periodicals, Inc. | en_US |
dc.subject.other | Magnetosheath | en_US |
dc.subject.other | Magnetosphere | en_US |
dc.subject.other | ULF | en_US |
dc.subject.other | Magnetopause | en_US |
dc.subject.other | Waves | en_US |
dc.title | Magnetospheric “magic” frequencies as magnetopause surface eigenmodes | en_US |
dc.type | Article | en_US |
dc.rights.robots | IndexNoFollow | en_US |
dc.subject.hlbsecondlevel | Geological Sciences | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/100327/1/grl50979.pdf | |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/100327/2/text01.pdf | |
dc.identifier.doi | 10.1002/grl.50979 | en_US |
dc.identifier.source | Geophysical Research Letters | en_US |
dc.identifier.citedreference | Samson, J. C., B. G. Harrold, J. M. Ruohoniemi, R. A. Greenwald, and A. D. M. Walker ( 1992 ), Field line resonances associated with MHD wave guides in the magnetosphere, Geophys. Res. Lett., 19, 441 – 444, doi: 10.1029/92GL00116. | en_US |
dc.identifier.citedreference | Kepko, L., and H. E. Spence ( 2003 ), Observations of discrete, global magnetospheric oscillations directly driven by solar wind density variations, J. Geophys. Res., 108, 1257, doi: 10.1029/2002JA009676. | en_US |
dc.identifier.citedreference | Kepko, L., H. E. Spence, and H. J. Singer ( 2002 ), ULF waves in the solar wind as direct drivers of magnetospheric pulsations, Geophys. Res. Lett., 29, 1197, doi: 10.1029/2001GL014405. | en_US |
dc.identifier.citedreference | Kivelson, M. G., and D. J. Southwood ( 1985 ), Resonant ULF waves: A new interpretation, Geophys. Res. Lett., 12, 49 – 52, doi: 10.1029/GL012i001p00049. | en_US |
dc.identifier.citedreference | Le, G., and C. T. Russell ( 1992 ), A study of ULF wave morphology—I: ULF foreshock boundary, Planet. Space Sci., 40, 1203 – 1213, doi: 10.1016/0032‐0633(92)90077‐2. | en_US |
dc.identifier.citedreference | Lee, D.‐H., and R. L. Lysak ( 1989 ), Magnetospheric ULF wave coupling in the dipole model: The impulsive excitation, J. Geophys. Res., 94, 17,097 – 17,103, doi: 10.1029/JA094iA12p17097. | en_US |
dc.identifier.citedreference | McFadden, J. P., C. W. Carlson, D. Larson, M. Ludlam, R. Abiad, B. Elliott, P. Turin, M. Marckwordt, and V. Angelopoulos ( 2008a ), The THEMIS ESA plasma instrument and in‐flight calibration, Space Sci. Rev., 141, 277 – 302, doi: 10.1007/s11214‐008‐9440‐2. | en_US |
dc.identifier.citedreference | McFadden, J. P., C. W. Carlson, J. Bonnell, F. Mozer, V. Angelopoulos, K. H. Glassmeier, and U. Auster ( 2008b ), THEMIS ESA first science results and performance issues, Space Sci. Rev., 141, 447 – 508, doi: 10.1007/s11214‐008‐9433‐1. | en_US |
dc.identifier.citedreference | Menk, F. W. ( 2011 ), Magnetospheric ULF waves: A review, in The Dynamic Magnetosphere, edited by W. Lui and M. Fujimoto, pp. 223 – 256, IAGA Special Sopron Book Series, Springer‐Verlag Berlin, Dordrecht, The Netherlands, doi: 10.1007/978‐94‐007‐0501‐2_13. | en_US |
dc.identifier.citedreference | Plaschke, F., and K. H. Glassmeier ( 2011 ), Properties of standing Kruskal‐Schwarzschild‐modes at the magnetopause, Ann. Geophys., 29, 1793 – 1807, doi: 10.5194/angeo‐29‐1793‐2011. | en_US |
dc.identifier.citedreference | Plaschke, F., K.‐H. Glassmeier, H. U. Auster, O. D. Constantinescu, W. Magnes, V. Angelopoulos, D. G. Sibeck, and J. P. McFadden ( 2009 ), Standing Alfvén waves at the magnetopause, Geophys. Res. Lett., 36, L02104, doi: 10.1029/2008GL036411. | en_US |
dc.identifier.citedreference | Powell, K. G., P. L. Roe, T. J. Linde, T. I. Gombosi, and D. L. De Zeeuw ( 1999 ), A solution‐adaptive upwind scheme for ideal magnetohydrodynamics, J. Comput. Phys., 154, 284 – 309, doi: 10.1006/jcph.1999.6299. | en_US |
dc.identifier.citedreference | Shue, J.‐H., J.‐K. Chao, P. Song, J. P. McFadden, A. Suvorova, V. Angelopoulos, K. H. Glassmeier, and F. Plaschke ( 2009 ), Anomalous magnetosheath flows and distorted subsolar magnetopause for radial interplanetary magnetic fields, Geophys. Res. Lett., 36, L18112, doi: 10.1029/2009GL039842. | en_US |
dc.identifier.citedreference | Singer, H. J., and M. G. Kivelson ( 1979 ), The latitudinal structure of Pc5 waves in space: Magnetic and electric field observations, J. Geophys. Res., 84, 7213 – 7222, doi: 10.1029/JA084iA12p07213. | en_US |
dc.identifier.citedreference | Southwood, D. J. ( 1974 ), Some features of field line resonances in the magnetosphere, Planet. Space Sci., 22, 483 – 491, doi: 10.1016/0032‐0633(74)90078‐6. | en_US |
dc.identifier.citedreference | Takahashi, K., R. L. McPherron, and T. Terasawa ( 1984 ), Dependence of the spectrum of Pc 3–4 pulsations on the interplanetary magnetic field, J. Geophys. Res., 89, 2770 – 2780, doi: 10.1029/JA089iA05p02770. | en_US |
dc.identifier.citedreference | Torrence, C., and G. P. Compo ( 1998 ), A practical guide to wavelet analysis, Bull. Amer. Meteor. Soc., 79, 61 – 78, doi: 10.1175/1520‐0477(1998)079<0061:APGTWA>2.0.CO;2. | en_US |
dc.identifier.citedreference | Tsyganenko, N. A. ( 1995 ), Modeling the Earth's magnetospheric magnetic field confined within a realistic magnetopause, J. Geophys. Res., 100, 5599 – 5612, doi: 10.1029/94JA03193. | en_US |
dc.identifier.citedreference | Tsyganenko, N. A., and D. P. Stern ( 1996 ), Modeling the global magnetic field of the large‐scale Birkeland current systems, J. Geophys. Res., 101, 27,187 – 27,198, doi: 10.1029/96JA02735. | en_US |
dc.identifier.citedreference | Tu, J., P. Song, B. W. Reinisch, and J. L. Green ( 2007 ), Smooth electron density transition from plasmasphere to the subauroral region, J. Geophys. Res., 112, A05227, doi: 10.1029/2007JA012298. | en_US |
dc.identifier.citedreference | Viall, N. M., L. Kepko, and H. E. Spence ( 2009 ), Relative occurrence rates and connection of discrete frequency oscillations in the solar wind density and dayside magnetosphere, J. Geophys. Res., 114, A01201, doi: 10.1029/2008JA013334. | en_US |
dc.identifier.citedreference | Waters, C. L., K. Takahashi, D.‐H. Lee, and B. J. Anderson ( 2002 ), Detection of ultralow‐frequency cavity modes using spacecraft data, J. Geophys. Res., 107, 1284, doi: 10.1029/2001JA000224. | en_US |
dc.identifier.citedreference | Angelopoulos, V. ( 2008 ), The THEMIS mission, Space Sci. Rev., 141, 5 – 34, doi: 10.1007/s11214‐008‐9336‐1. | en_US |
dc.identifier.citedreference | Archer, M. O., and T. S. Horbury ( 2013 ), Magnetosheath dynamic pressure enhancements: Occurrence and typical properties, Ann. Geophys., 31, 319 – 331, doi: 10.5194/angeo‐31‐319‐2013. | en_US |
dc.identifier.citedreference | Archer, M. O., T. S. Horbury, and J. P. Eastwood ( 2012 ), Magnetosheath pressure pulses: Generation downstream of the bow shock from solar wind discontinuities, J. Geophys. Res., 117, A05228, doi: 10.1029/2011JA017468. | en_US |
dc.identifier.citedreference | Archer, M. O., T. S. Horbury, J. P. Eastwood, J. M. Weygand, and T. K. Yeoman ( 2013 ), Magnetospheric response to magnetosheath pressure pulses: A low pass filter effect, J. Geophys. Res. Space Physics, 118, doi: 10.1002/jgra.50519. | en_US |
dc.identifier.citedreference | Auster, H. U., et al. ( 2008 ), The THEMIS fluxgate magnetometer, Space Sci. Rev., 141, 235 – 264, doi: 10.1007/s11214‐008‐9365‐9. | en_US |
dc.identifier.citedreference | Chen, L., and A. Hasegawa ( 1974 ), A theory of long‐period magnetic pulsations: 2. Impulse excitation of surface eigenmode, J. Geophys. Res., 79, 1033 – 1037, doi: 10.1029/JA079i007p01033. | en_US |
dc.identifier.citedreference | Clausen, L. B. N., T. K. Yeoman, R. C. Fear, R. Behlke, E. A. Lucek, and M. J. Engebretson ( 2009 ), First simultaneous measurements of waves generated at the bow shock in the solar wind, the magnetosphere and on the ground, Ann. Geophys., 27, 357 – 371, doi: 10.5194/angeo‐27‐357‐2009. | en_US |
dc.identifier.citedreference | Francia, P., and U. Villante ( 1997 ), Some evidence of ground power enhancements at frequencies of global magnetospheric modes at low latitude, Ann. Geophys., 15, 17 – 23, doi: 10.1007/s00585‐997‐0017‐2. | en_US |
dc.identifier.citedreference | Hartinger, M., M. B. Moldwin, V. Angelopoulos, K. Takahashi, H. J. Singer, R. R. Anderson, Y. Nishimura, and J. R. Wygant ( 2010 ), Pc5 wave power in the quiet‐time plasmasphere and trough: CRRES observations, Geophys. Res. Lett., 37, L07107, doi: 10.1029/2010GL042475. | en_US |
dc.identifier.citedreference | Hartinger, M. D., V. Angelopoulos, M. B. Moldwin, K. Takahashi, and L. B. N. Clausen ( 2013 ), Statistical study of global modes outside the plasmasphere, J. Geophys. Res. Space Physics, 118, 804 – 822, doi: 10.1002/jgra.50140. | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
Files in this item
Remediation of Harmful Language
The University of Michigan Library aims to describe library materials in a way that respects the people and communities who create, use, and are represented in our collections. Report harmful or offensive language in catalog records, finding aids, or elsewhere in our collections anonymously through our metadata feedback form. More information at Remediation of Harmful Language.
Accessibility
If you are unable to use this file in its current format, please select the Contact Us link and we can modify it to make it more accessible to you.