Effects of crustal field rotation on the solar wind plasma interaction with Mars
dc.contributor.author | Ma, Yingjuan | en_US |
dc.contributor.author | Fang, Xiaohua | en_US |
dc.contributor.author | Russell, Christopher T. | en_US |
dc.contributor.author | Nagy, Andrew F. | en_US |
dc.contributor.author | Toth, Gabor | en_US |
dc.contributor.author | Luhmann, Janet G. | en_US |
dc.contributor.author | Brain, Dave A. | en_US |
dc.contributor.author | Dong, Chuanfei | en_US |
dc.date.accessioned | 2014-11-04T16:35:56Z | |
dc.date.available | WITHHELD_12_MONTHS | en_US |
dc.date.available | 2014-11-04T16:35:56Z | |
dc.date.issued | 2014-10-16 | en_US |
dc.identifier.citation | Ma, Yingjuan; Fang, Xiaohua; Russell, Christopher T.; Nagy, Andrew F.; Toth, Gabor; Luhmann, Janet G.; Brain, Dave A.; Dong, Chuanfei (2014). "Effects of crustal field rotation on the solar wind plasma interaction with Mars." Geophysical Research Letters 41(19): 6563-6569. | en_US |
dc.identifier.issn | 0094-8276 | en_US |
dc.identifier.issn | 1944-8007 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/109356 | |
dc.description.abstract | The crustal remnant field on Mars rotates with the planet at a period of 24 h 37 min, constantly varying the magnetic field configuration interacting with the solar wind. Until now, there has been no self‐consistent modeling investigation on how this varying magnetic field affects the solar wind plasma interaction. Here we include the rotation of this localized crustal field in a multispecies single‐fluid MHD model of Mars and simulate an entire day of solar wind interaction under normal solar wind conditions. The MHD model results are compared with Mars Global Surveyor (MGS) magnetic field observations and show very close agreement, especially for the field strength along almost all of the 12 orbits on the day simulated. Model results also show that the ion escape rates slowly vary with rotation, generally anticorrelating with the strength of subsolar magnetic crustal sources, with some time delay. In addition, it is found that in the intense crustal field regions, the densities of heavy ion components enhance significantly along the MGS orbit, implying strong influence of the crustal field on the ionospheric structures. Key Points Model results closely agree with MGS observations Ion escape rates slowly vary with rotation Crustal field has strong influence on the ionospheric structures | en_US |
dc.publisher | Wiley Periodicals, Inc. | en_US |
dc.subject.other | Rotation | en_US |
dc.subject.other | Mars | en_US |
dc.subject.other | Crustal Field | en_US |
dc.title | Effects of crustal field rotation on the solar wind plasma interaction with Mars | 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/2027.42/109356/1/grl52074.pdf | |
dc.identifier.doi | 10.1002/2014GL060785 | en_US |
dc.identifier.source | Geophysical Research Letters | en_US |
dc.identifier.citedreference | Acuna, M. H., et al. ( 1999 ), Global distribution of crustal magnetization discovered by the Mars global surveyor MAG/ER experiment, Science, 284, 790 – 793. | en_US |
dc.identifier.citedreference | Arkani‐Hamed, J. ( 2001 ), A 50‐degree spherical harmonic model of the magnetic field of Mars, J. Geophys. Res., 106, 23,197 – 23,208, doi: 10.1029/2000JE001365. | en_US |
dc.identifier.citedreference | Acuna, M. H., et al. ( 1998 ), Magnetic field and plasma observations at Mars: Initial results of the Mars Global Surveyor mission, Science, 279, 1676 – 1680. | en_US |
dc.identifier.citedreference | Nagy, A., et al. ( 2004 ), The plasma environment of Mars, Space Sci. Rev., 111, 33 – 114. | en_US |
dc.identifier.citedreference | Modolo, R., G. M. Chanteur, and E. Dubinin ( 2012 ), Dynamic Martian magnetosphere: Transient twist induced by a rotation of the IMF, Geophys. Res. Lett., 39, L01106, doi: 10.1029/2011GL049895. | en_US |
dc.identifier.citedreference | Ma, Y.‐J., and A. F. Nagy ( 2007 ), Ion escape fluxes from Mars, Geophys. Res. Lett., 34, L08201, doi: 10.1029/2006GL029208. | en_US |
dc.identifier.citedreference | Ma, Y., A. F. Nagy, I. V. Sokolov, and K. C. Hansen ( 2004 ), Three‐dimensional, multispecies, high spatial resolution MHD studies of the solar wind interaction with Mars, J. Geophys. Res., 109, A07211, doi: 10.1029/2003JA010367. | en_US |
dc.identifier.citedreference | Ma, Y. J., X. Fang, A. F. Nagy, C. T. Russell, and G. Toth ( 2014 ), Martian ionospheric responses to dynamic pressure enhancements in the solar wind, J. Geophys. Res. Space Physics, 119, 1272 – 1286, doi: 10.1002/2013JA019402. | en_US |
dc.identifier.citedreference | Lundin, R., S. Barabash, M. Holmström, H. Nilsson, Y. Futaana, R. Ramstad, M. Yamauchi, E. Dubinin, and M. Fraenz ( 2013 ), Solar cycle effects on the ion escape from Mars, Geophys. Res. Lett., 40, 6028 – 6032, doi: 10.1002/2013GL058154. | en_US |
dc.identifier.citedreference | Lundin, R., S. Barabash, M. Yamauchi, H. Nilsson, and D. Brain ( 2011 ), On the relation between plasma escape and the martian crustal magnetic field, Geophys. Res. Lett., 38, L02102, doi: 10.1029/2010GL046019. | en_US |
dc.identifier.citedreference | Ledvina, S. A., Y. J. Ma, and E. Kallio ( 2008 ), Modeling and simulating flowing plasmas and related phenomena, Space Sci. Rev., doi: 10.1007/s11214-008-9384-6. | en_US |
dc.identifier.citedreference | Kallio, E., J.‐Y. Chaufray, R. Modolo, D. Snowden, and R. Winglee ( 2011 ), Modeling of Venus, Mars, and Titan, Space Sci. Rev., 162 ( 1–4 ), 267 – 307, doi: 10.1007/s11214-011-9814-8. | en_US |
dc.identifier.citedreference | Nilsson, H., et al. ( 2011 ), Heavy ion escape from Mars, influence from solar wind conditions and crustal magnetic fields, Icarus, 215 ( 2 ), 475 – 484, doi: 10.1016/j.icarus.2011.08.003. | en_US |
dc.identifier.citedreference | Powell, K. G., P. L. Roe, T. J. Linde, T. I. Gombosi, and D. L. DeZeeuw ( 1999 ), A solution‐adaptive upwind scheme for ideal magnetohydrodynamics, J. Comp. Phys., 154, 284 – 309. | en_US |
dc.identifier.citedreference | Toth, G., et al. ( 2012 ), Adaptive numerical algorithms in space weather modeling, J. Comput. Phys., 231 ( 3 ), 870 – 903, doi: 10.1016/j.jcp.2011.02.006. | en_US |
dc.identifier.citedreference | Fang, X., M. W. Liemohn, A. F. Nagy, J. Luhmann, and Y. Ma ( 2010 ), On the effect of the martian crustal magnetic field on atmospheric erosion, Icarus, 206, 130 – 138, doi: 10.1016/j.icarus.2009.01.012. | en_US |
dc.identifier.citedreference | Crider, D. H., D. Vignes, A. M. Krymskii, T. K. Breus, N. F. Ness, D. L. Mitchell, J. A. Slavin, and M. H. Acuña ( 2003 ), A proxy for determining solar wind dynamic pressure at Mars using Mars Global Surveyor data, J. Geophys. Res., 108 ( A12 ), 1461, doi: 10.1029/2003JA009875. | en_US |
dc.identifier.citedreference | Connerney, J. E. P., M. H. Acuña, P. J. Wasilewski, N. F. Ness, H. Rème, C. Mazelle, D. Vignes, R. P. Lin, D. L. Mitchell, and P. A. Cloutier ( 1999 ), Magnetic lineations in the ancient crust of Mars, Science, 284, 794 – 798. | en_US |
dc.identifier.citedreference | Carlsson, E., et al. ( 2006 ), Mass composition of the escaping plasma at, Icarus, 182, 320 – 328, doi: 10.1016/j.icarus.2005.09.020. | en_US |
dc.identifier.citedreference | Brain, D. A., et al. ( 2010 ), A comparison of global models for the solar wind interaction with Mars, Icarus, 206 ( 1 ), 139 – 151, doi: 10.1016/j.icarus.2009.06.030. | en_US |
dc.identifier.citedreference | Brain, D. A., J. S. Halekas, R. Lillis, D. L. Mitchell, R. P. Lin, and D. H. Crider ( 2005 ), Variability of the altitude of the Martian sheath, Geophys. Res. Lett., 32, L18203, doi: 10.1029/2005GL023126. | en_US |
dc.identifier.citedreference | Brain, D. A. ( 2006 ), Mars Global Surveyor measurements of the Martian solar wind interaction, Space Sci. Rev., 126 ( January ), 77 – 112, doi: 10.1007/s11214-006-9122-x. | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
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