Show simple item record

Plasma pressure in Mercury's equatorial magnetosphere derived from MESSENGER Magnetometer observations

dc.contributor.authorKorth, Hajeen_US
dc.contributor.authorAnderson, Brian J.en_US
dc.contributor.authorRaines, Jim M.en_US
dc.contributor.authorSlavin, James A.en_US
dc.contributor.authorZurbuchen, Thomas H.en_US
dc.contributor.authorJohnson, Catherine L.en_US
dc.contributor.authorPurucker, Michael E.en_US
dc.contributor.authorWinslow, Reka M.en_US
dc.contributor.authorSolomon, Sean C.en_US
dc.contributor.authorMcNutt, Ralph L.en_US
dc.date.accessioned2013-01-03T19:42:07Z
dc.date.available2013-01-03T19:42:07Z
dc.date.issued2011-11en_US
dc.identifier.citationKorth, Haje; Anderson, Brian J.; Raines, Jim M.; Slavin, James A.; Zurbuchen, Thomas H.; Johnson, Catherine L.; Purucker, Michael E.; Winslow, Reka M.; Solomon, Sean C.; McNutt, Ralph L. (2011). "Plasma pressure in Mercury's equatorial magnetosphere derived from MESSENGER Magnetometer observations." Geophysical Research Letters 38(22): n/a-n/a. <http://hdl.handle.net/2027.42/95264>en_US
dc.identifier.issn0094-8276en_US
dc.identifier.issn1944-8007en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/95264
dc.publisherWiley Periodicals, Inc.en_US
dc.publisherImp. Coll. Pressen_US
dc.subject.otherPlasmaen_US
dc.subject.otherMagnetosphereen_US
dc.subject.otherMagnetic Fielden_US
dc.subject.otherMercuryen_US
dc.titlePlasma pressure in Mercury's equatorial magnetosphere derived from MESSENGER Magnetometer observationsen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelGeological Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/95264/1/grl28621-sup-0002-txts01.pdf
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/95264/2/grl28621.pdf
dc.identifier.doi10.1029/2011GL049451en_US
dc.identifier.sourceGeophysical Research Lettersen_US
dc.identifier.citedreferenceTrávníček, P. M., P. Hellinger, and D. Schriver ( 2007 ), Structure of Mercury's magnetosphere for different pressure of the solar wind: Three‐dimensional hybrid simulations, Geophys. Res. Lett., 34, L05104, doi: 10.1029/2006GL028518.en_US
dc.identifier.citedreferenceBorovsky, J. E., R. C. Elphic, H. O. Funsten, and M. F. Thomsen ( 1997 ), The Earth's plasma sheet as a laboratory for flow turbulence in high‐beta MHD, J. Plasma Phys., 57, 1 – 34, doi: 10.1017/S0022377896005259.en_US
dc.identifier.citedreferenceBüchner, J., and L. M. Zelenyi ( 1989 ), Regular and chaotic charged‐particle motion in magnetotail‐like field reversals: 1. Basic theory of trapped motion, J. Geophys. Res., 94, 11,821 – 11,842, doi: 10.1029/JA094iA09p11821.en_US
dc.identifier.citedreferenceDelcourt, D. C., and R. F. Martin ( 1994 ), Application of the centrifugal impulse model to particle motion in the near‐Earth magnetotail, J. Geophys. Res., 99, 23,583 – 23,590, doi: 10.1029/94JA01845.en_US
dc.identifier.citedreferenceDelcourt, D. C., S. Grimald, F. Leblanc, J. J. Berthelier, A. Millilo, A. Mura, S. Orsini, and T. E. Moore ( 2003 ), A quantitative model of the planetary Na + contribution to Mercury's magnetosphere, Ann. Geophys., 21, 1723 – 1736, doi: 10.5194/angeo‐21‐1723‐2003.en_US
dc.identifier.citedreferenceDungey, J. W. ( 1961 ), Interplanetary magnetic field and auroral zones, Phys. Rev. Lett., 6, 47 – 48, doi: 10.1103/PhysRevLett.6.47.en_US
dc.identifier.citedreferenceFriedel, R. H. W., H. Korth, M. G. Henderson, M. F. Thomsen, and J. D. Scudder ( 2001 ), Plasma sheet access to the inner magnetosphere, J. Geophys. Res., 106, 5845 – 5858, doi: 10.1029/2000JA003011.en_US
dc.identifier.citedreferenceKabin, K., T. I. Gombosi, D. L. DeZeeuw, and K. G. Powell ( 2000 ), Interaction of Mercury with the solar wind, Icarus, 143, 397 – 406, doi: 10.1006/icar.1999.6252.en_US
dc.identifier.citedreferenceKallio, E., and P. Janhunen ( 2003 ), Modelling the solar wind interaction with Mercury by a quasi‐neutral hybrid model, Ann. Geophys., 21, 2133 – 2145, doi: 10.5194/angeo‐21‐2133‐2003.en_US
dc.identifier.citedreferenceKorth, H., M. F. Thomsen, J. E. Borovsky, and D. J. McComas ( 1999 ), Plasma sheet access to geosynchronous orbit, J. Geophys. Res., 104, 25,047 – 25,061, doi: 10.1029/1999JA900292.en_US
dc.identifier.citedreferenceMura, A., S. Orsini, A. Milillo, D. Delcourt, S. Massetti, and E. De Angelis ( 2005 ), Dayside H + circulation at Mercury and neutral particle emission, Icarus, 175, 305 – 319, doi: 10.1016/j.icarus.2004.12.010.en_US
dc.identifier.citedreferenceNess, N. F., K. W. Behannon, R. P. Lepping, and Y. C. Whang ( 1975 ), Magnetic field of Mercury, 1, J. Geophys. Res., 80, 2708 – 2716, doi: 10.1029/JA080i019p02708.en_US
dc.identifier.citedreferenceOhtani, S., M. Nose, S. P. Christon, and A. T. Y. Lui ( 2011 ), Energetic O + and H + ions in the plasma sheet: Implications for the transport of ionospheric ions, J. Geophys. Res., 116, A10211, doi: 10.1029/2011JA016532.en_US
dc.identifier.citedreferenceSchulz, M., and L. J. Lanzerotti ( 1974 ), Particle Diffusion in the Radiation Belts, Phys. Chem. Space, vol. 7, 215 pp., Springer, New York.en_US
dc.identifier.citedreferenceSlavin, J. A., et al. ( 2009 ), MESSENGER observations of magnetic reconnection in Mercury's magnetosphere, Science, 324, 606 – 610, doi: 10.1126/science.1172011.en_US
dc.identifier.citedreferenceSlavin, J. A., et al. ( 2010 ), MESSENGER observations of extreme loading and unloading of Mercury's magnetic tail, Science, 329, 665 – 668, doi: 10.1126/science.1188067.en_US
dc.identifier.citedreferenceStern, D. P. ( 1975 ), The motion of a proton in the equatorial magnetosphere, J. Geophys. Res., 80, 595 – 599, doi: 10.1029/JA080i004p00595.en_US
dc.identifier.citedreferenceTrávníček, P. M., P. Hellinger, D. Schriver, D. Herčík, J. A. Slavin, and B. J. Anderson ( 2009 ), Kinetic instabilities in Mercury's magnetosphere: Three‐dimensional simulation results, Geophys. Res. Lett., 36, L07104, doi: 10.1029/2008GL036630.en_US
dc.identifier.citedreferenceTrávníček, P. M., D. Schriver, P. Hellinger, D. Herčík, B. J. Anderson, M. Sarantos, and J. A. Slavin ( 2010 ), Mercury's magnetosphere‐solar wind interaction for northward and southward interplanetary magnetic field: Hybrid simulation results, Icarus, 209, 11 – 22, doi: 10.1016/j.icarus.2010.01.008.en_US
dc.identifier.citedreferenceVolland, H. ( 1973 ), Semiempirical model of large‐scale magnetospheric electric fields, J. Geophys. Res., 78, 171 – 180, doi: 10.1029/JA078i001p00171.en_US
dc.identifier.citedreferenceVolland, H. ( 1975 ), Models of global electric fields within the magnetosphere, Ann. Geophys., 31, 159 – 173.en_US
dc.identifier.citedreferenceVolland, H. ( 1978 ), Model of magnetospheric electric convection field, J. Geophys. Res., 83, 2695 – 2699, doi: 10.1029/JA083iA06p02695.en_US
dc.identifier.citedreferenceWang, C. P., L. R. Lyons, J. M. Weygand, T. Nagai, and R. W. McEntire ( 2006 ), Equatorial distributions of the plasma sheet ions, their electric and magnetic drifts, and magnetic fields under different interplanetary magnetic field B z conditions, J. Geophys. Res., 111, A04215, doi: 10.1029/2005JA011545.en_US
dc.identifier.citedreferenceWhipple, E. C. ( 1978 ), ( U, B, K ) coordinates: A natural system for studying magnetospheric convection, J. Geophys. Res., 83, 4318 – 4326, doi: 10.1029/JA083iA09p04318.en_US
dc.identifier.citedreferenceWing, S., and P. T. Newell ( 1998 ), Central plasma sheet ion properties as inferred from ionospheric observations, J. Geophys. Res., 103, 6785 – 6800, doi: 10.1029/97JA02994.en_US
dc.identifier.citedreferenceYagi, M., K. Seki, Y. Matsumoto, D. C. Delcourt, and F. Leblanc ( 2010 ), Formation of a sodium ring in Mercury's magnetosphere, J. Geophys. Res., 115, A10253, doi: 10.1029/2009JA015226.en_US
dc.identifier.citedreferenceZurbuchen, T. H., et al. ( 2011 ), MESSENGER observations of the spatial distribution of planetary ions near Mercury, Science, 333, 1862 – 1865, doi: 10.1126/science.1211302.en_US
dc.identifier.citedreferenceAlexeev, I. I., E. S. Belenkaya, S. Y. Bobrovnikov, J. A. Slavin, and M. Sarantos ( 2008 ), Paraboloid model of Mercury's magnetosphere, J. Geophys. Res., 113, A12210, doi: 10.1029/2008JA013368.en_US
dc.identifier.citedreferenceAlexeev, I. I., et al. ( 2010 ), Mercury's magnetospheric magnetic field after the first two MESSENGER flybys, Icarus, 209, 23 – 39, doi: 10.1016/j.icarus.2010.01.024.en_US
dc.identifier.citedreferenceAnderson, B. J., M. H. Acuña, D. A. Lohr, J. Scheifele, A. Raval, H. Korth, and J. A. Slavin ( 2007 ), The Magnetometer instrument on MESSENGER, Space Sci. Rev., 131, 417 – 450, doi: 10.1007/s11214‐007‐9246‐7.en_US
dc.identifier.citedreferenceAnderson, B. J., C. L. Johnson, H. Korth, M. E. Purucker, R. M. Winslow, J. A. Slavin, S. C. Solomon, R. L. McNutt Jr., J. M. Raines, and T. H. Zurbuchen ( 2011 ), The global magnetic field of Mercury from MESSENGER orbital observations, Science, 333, 1859 – 1862, doi: 10.1126/science.1211001.en_US
dc.identifier.citedreferenceAndrews, G. B., et al. ( 2007 ), The Energetic Particle and Plasma Spectrometer instrument on the MESSENGER spacecraft, Space Sci. Rev., 131, 523 – 556, doi: 10.1007/s11214‐007‐9272‐5.en_US
dc.identifier.citedreferenceBaumjohann, W., and R. A. Treumann ( 1997 ), Basic Space Plasma Physics, 329 pp., Imp. Coll. Press, London.en_US
dc.identifier.citedreferenceBenna, M., et al. ( 2010 ), Modeling of the magnetosphere of Mercury at the time of the first MESSENGER flyby, Icarus, 209, 3 – 10, doi: 10.1016/j.icarus.2009.11.036.en_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


Files in this item

Show simple item record

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.