Influence of the Interplanetary Convective Electric Field on the Distribution of Heavy Pickup Ions Around Mars
dc.contributor.author | Johnson, B. C. | |
dc.contributor.author | Liemohn, M. W. | |
dc.contributor.author | Fránz, M. | |
dc.contributor.author | Ramstad, R. | |
dc.contributor.author | Stenberg Wieser, G. | |
dc.contributor.author | Nilsson, H. | |
dc.date.accessioned | 2018-03-07T18:26:06Z | |
dc.date.available | 2019-03-01T21:00:18Z | en |
dc.date.issued | 2018-01 | |
dc.identifier.citation | Johnson, B. C.; Liemohn, M. W.; Fránz, M. ; Ramstad, R.; Stenberg Wieser, G.; Nilsson, H. (2018). "Influence of the Interplanetary Convective Electric Field on the Distribution of Heavy Pickup Ions Around Mars." Journal of Geophysical Research: Space Physics 123(1): 473-484. | |
dc.identifier.issn | 2169-9380 | |
dc.identifier.issn | 2169-9402 | |
dc.identifier.uri | https://hdl.handle.net/2027.42/142551 | |
dc.description.abstract | This study obtains a statistical representation of 2–15 keV heavy ions outside of the Martian‐induced magnetosphere and depicts their organization by the solar wind convective electric field (ESW). The overlap in the lifetime of Mars Global Surveyor (MGS) and Mars Express (MEX) provides a period of nearly three years during which magnetometer data from MGS can be used to estimate the direction of ESW in order to better interpret MEX ion data. In this paper we use MGS estimates of ESW to express MEX ion measurements in Mars‐Sun‐Electric field (MSE) coordinates. A new methodological technique used in this study is the limitation of the analysis to a particular instrument mode for which the overlap between proton contamination and plume observations is rare. This allows for confident energetic heavy ion identification outside the induced magnetosphere boundary. On the dayside, we observe high count rates of 2–15 keV heavy ions more frequently in the +ESW hemisphere (+ZMSE) than in the −ESW hemisphere, but on the nightside the reverse asymmetry was found. The results are consistent with planetary origin ions being picked up by the solar wind convective electric field. Though a field of view hole hinders quantification of plume fluxes and velocity space, this new energetic heavy ion identification technique means that Mars Express should prove useful in expanding the time period available to assess general plume loss variation with drivers.Plain Language SummaryThe location and flow direction of oxygen escaping Mars’ atmosphere is organized by a global‐scale electric field associated with the Sun’s flowing magnetic field. While the Mars Express (MEX) satellite is less well equipped than Mars Atmosphere and Volatile Evolution (MAVEN) to estimate exact flux values of ions accelerated by this electric field, our demonstration that MEX can see this population statistically opens a new window of time (pre‐MAVEN) to studies of the variability of this atmospheric escape channel.Key PointsMars Express heavy ion data outside the magnetic boundary show a statistical asymmetry consistent with other energetic plume studiesThe energetic plume is more prevalent on the dayside (i.e., X > 0), while for X < 0 higher count rates in the +ESW direction were not seenFor a specific instrument setting, overlap between proton contamination and the plume is rare, allowing for confident plume identification | |
dc.publisher | SP‐1240, ESA Publications Division | |
dc.publisher | Wiley Periodicals, Inc. | |
dc.subject.other | ion escape | |
dc.subject.other | convective electric field | |
dc.subject.other | Mars Express | |
dc.subject.other | MEX data analysis | |
dc.subject.other | Mars ion loss | |
dc.title | Influence of the Interplanetary Convective Electric Field on the Distribution of Heavy Pickup Ions Around Mars | |
dc.type | Article | en_US |
dc.rights.robots | IndexNoFollow | |
dc.subject.hlbsecondlevel | Astronomy and Astrophysics | |
dc.subject.hlbtoplevel | Science | |
dc.description.peerreviewed | Peer Reviewed | |
dc.description.bitstreamurl | https://deepblue.lib.umich.edu/bitstream/2027.42/142551/1/jgra53999.pdf | |
dc.description.bitstreamurl | https://deepblue.lib.umich.edu/bitstream/2027.42/142551/2/jgra53999_am.pdf | |
dc.identifier.doi | 10.1002/2017JA024463 | |
dc.identifier.source | Journal of Geophysical Research: Space Physics | |
dc.identifier.citedreference | Luhmann, J. G., & Schwingenschuh, K. ( 1990 ). A model of the energetic ion environment of Mars. Journal of Geophysical Research, 95 ( A2 ), 939 – 945. https://doi.org/10.1029/JA095iA02p00939 | |
dc.identifier.citedreference | Edberg, N. J. T., Auster, U., Barabash, S., Bößwetter, A., Brain, D. A., Burch, J. L., … Trotignon, J. G. ( 2009 ). Rosetta and Mars Express observations of the influence of high solar wind pressure on the Martian plasma environment. Annales de Geophysique, 27 ( 12 ), 4533 – 4545. https://doi.org/10.5194/angeo‐27‐4533‐2009 | |
dc.identifier.citedreference | Fang, X., Liemohn, M. W., Nagy, A. F., Ma, Y., De Zeeuw, D. L., Kozyra, J. U., & Zurbuchen, T. ( 2008 ). Pickup oxygen ion distribution around Mars. Journal of Geophysical Research, 113, A02210. https://doi.org/10.1029/2007JA012736 | |
dc.identifier.citedreference | Fedorov, A., Budnik, E., Sauvaud, J. A., Mazelle, C., Barabash, S., Lundin, R., … Dierker, C. ( 2006 ). Structure of the Martian wake. Icarus, 182 ( 2 ), 329 – 336. https://doi.org/10.1016/j.icarus.2005.09.021 | |
dc.identifier.citedreference | Fedorov, A., Ferrier, C., Sauvaud, J. A., Barabash, S., Zhang, T. L., Mazelle, C., … Bochsler, P. ( 2008 ). Comparative analysis of Venus and Mars magnetotails. Planetary and Space Science, 56 ( 6 ), 812 – 817. https://doi.org/10.1016/j.pss.2007.12.012 | |
dc.identifier.citedreference | Fraenz, M., Dubinin, E., Andrews, D., Barabash, S., Nilsson, H., & Fedorov, A. ( 2015 ). Cold ion escape from the Martian ionosphere. Planetary and Space Science, 119, 92 – 102. https://doi.org/10.1016/j.pss.2015.07.012 | |
dc.identifier.citedreference | Harnett, E. M., & Winglee, R. M. ( 2006 ). Three‐dimensional multifluid simulations of ionospheric loss at Mars from nominal solar wind conditions to magnetic cloud events. Journal of Geophysical Research, 111, A09213. https://doi.org/10.1029/2006JA011724 | |
dc.identifier.citedreference | Kallio, E., & Koskinen, H. ( 1999 ). A test particle simulation of the motion of oxygen ions and the solar wind protons. Journal of Geophysical Research, 104 ( A1 ), 557 – 579. https://doi.org/10.1029/1998JA900043 | |
dc.identifier.citedreference | Kallio, E., Koskinen, H., Barabash, S., Nairn, C. M. C., & Schwingenschuh, K. ( 1995 ). Oxygen outflow in the Martian magnetotail. Geophysical Research Letters, 22 ( 18 ), 2449 – 2452. https://doi.org/10.1029/95GL02474 | |
dc.identifier.citedreference | Kallio, E., Fedorov, A., Barabash, S., Janhunen, R., Koskinen, H., Schmidt, W., … Sharber, J. R. ( 2006 ). Energisation of O+ and O2+ ions at Mars: An analysis of a 3‐D quasi‐neutral hybrid model simulation. Space Science Reviews, 126, 39 – 62. | |
dc.identifier.citedreference | Liemohn, M. W., Ma, Y., Frahm, R. A., Fang, X., Kozyra, J. U., Nagy, A. F., … Lundin, R. ( 2007 ). Mars global MHD predictions of magnetic connectivity between the dayside ionosphere and the magnetospheric flanks. Space Science Reviews, 126 ( 1‐4 ), 63 – 76. https://doi.org/10.1007/s11214‐006‐9116‐8 | |
dc.identifier.citedreference | Liemohn, M. W., Curry, S. M., Fang, X., & Ma, Y. ( 2013 ). Comparison of high‐altitude production and ionospheric outflow contributions to O + loss at Mars. Journal of Geophysical Research: Space Physics, 118, 4093 – 4107. https://doi.org/10.1002/jgra.50388 | |
dc.identifier.citedreference | Liemohn, M. W., Johnson, B. C., Fränz, M., & Barabash, S. ( 2014 ). Mars Express observations of high altitude planetary ion beams and their relation to the “energetic plume” loss channel. Journal of Geophysical Research, 119, 9702 – 9713. https://doi.org/10.1002/2014JA019994 | |
dc.identifier.citedreference | Luhmann, J. G., Ma, Y.‐J., Brain, D. A., Ulusen, D., Lillis, R. J., Halekas, J. S., & Espley, J. R. ( 2015 ). Solar wind interaction effects on the magnetic fields around Mars: Consequences for interplanetary and crustal field measurements. Planetary and Space Science, 117, 15 – 23. https://doi.org/10.1016/j.pss.2015.05.004 | |
dc.identifier.citedreference | Lundin, R., & Dubinin, E. M. ( 1992 ). Phobos‐2 results on the ionospheric plasma escape from Mars. Advances in Space Research, 12 ( 9 ), 255 – 263. https://doi.org/10.1016/0273‐1177(92)90338‐X | |
dc.identifier.citedreference | Lundin, R., Barabash, S., Andersson, H., Holmström, M., Grigoriev, A., Yamauchi, M., … Bochsler, P. ( 2004 ). Solar wind‐induced atmospheric erosion at Mars: First results from ASPREA‐3 on Mars Express. Science, 305, 1993 – 1936. | |
dc.identifier.citedreference | Lundin, R., Barabash, S., Holmström, M., Nilsson, H., Yamauchi, M., Fraenz, M., & Dubinin, E. M. ( 2008 ). A comet‐like escape of ionospheric plasma from Mars. Geophysical Research Letters, 35, L18203. https://doi.org/10.1029/2008GL034811 | |
dc.identifier.citedreference | Lundin, R., Barabash, S., Yamauchi, M., Nilsson, H., & Brain, D. ( 2011 ). On the relation between plasma escape and the Martian crustal magnetic field. Geophysical Research Letters, 38, L02102. https://doi.org/10.1029/2010GL046019 | |
dc.identifier.citedreference | Modolo, R., Chanteur, G. M., Dubinin, E., & Matthews, A. P. ( 2005 ). Influence of the solar EUV flux on the Martian plasma environment. Annales de Geophysique, 23 ( 2 ), 433 – 444. https://doi.org/10.5194/angeo‐23‐433‐2005 | |
dc.identifier.citedreference | Najib, D., Nagy, A. F., Tth, G., & Ma, Y. ( 2011 ). Three‐dimensional, multifluid, high spatial resolution mhd model studies of the solar wind interaction with mars. Journal of Geophysical Research, 116, A05204. https://doi.org/10.1029/2010JA016272 | |
dc.identifier.citedreference | Nilsson, H., Edberg, N. J. T., Stenberg, G., Barabash, S., Holmstrm, M., Futaana, Y., … Fedorov, A. ( 2011 ). Heavy ion escape from Mars, influence from solar wind conditions and crustal magnetic fields. Icarus, 215 ( 2 ), 475 – 484. https://doi.org/10.1016/j.icarus.2011.08.003 | |
dc.identifier.citedreference | Nilsson, H., Stenberg, G., Futaana, S., Holmstrom, M., Barabash, S., Lundin, R., … Fedorov, A. ( 2012 ). Ion distributions in the vicinity of Mars: Signatures of heating and acceleration processes. Earth, Planets and Space, 64 ( 2 ), 135 – 148. https://doi.org/10.5047/eps.2011.04.011 | |
dc.identifier.citedreference | Vignes, D., Mazelle, C., Rme, H., Acufia, M. H., Connerney, J. E. P., Mitchell, D. L., … Univer‐, R. ( 2000 ). Shapes of the bow shock and the magnetic pile‐up boundary from the observations of the MAG/ER experiment onboard Mars Global Surveyor. Geophysical Research Letters, 27 ( 1 ), 49 – 52. https://doi.org/10.1029/1999GL010703 | |
dc.identifier.citedreference | Wang, X. D., Barabash, S., Futaana, Y., Grigoriev, A., & Wurz, P. ( 2013 ). Directionality and variability of energetic neutral hydrogen fluxes observed by Mars Express. Journal of Geophysical Research: Space Physics, 118, 7635 – 7642. https://doi.org/10.1002/2013JA018876 | |
dc.identifier.citedreference | Xu, S., Mitchell, D., Liemohn, M., Fang, X., Ma, Y., Luhmann, J., … Jakosky, B. ( 2017 ). Martian low‐altitude magnetic topology deduced from MAVEN/SWEA observations. Journal of Geophysical Research: Space Physics, 122, 1831 – 1852. https://doi.org/10.1002/2016JA023467 | |
dc.identifier.citedreference | Barabash, S., Dubinin, E., Pisarenko, N., Lundin, R., & Russell, C. T. ( 1991 ). Picked‐up protons near Mars‐PHOBOS observations. Geophysical Research Letters, 18 ( 10 ), 1805 – 1808. https://doi.org/10.1029/91GL02082 | |
dc.identifier.citedreference | Barabash, S., Lundin, R., Andersson, H., Gimholt, J., Holmstrom, M., Norberg, O., … Bochsler, P. ( 2004 ). ASPERA‐3: Analyser of Space Plasmas and Energetic Ions for Mars Express. In Mars Express: The Scientific Payload (pp. 121 – 139 ). Noordwijk, Netherlands: SP‐1240, ESA Publications Division. | |
dc.identifier.citedreference | Barabash, S., Lundin, R., Andersson, H., Brinkfeldt, K., Grigoriev, A., Gunell, H., … Thocaven, J.‐J. ( 2006 ). The Analyzer of Space Plasmas and Energetic Atoms (ASPERA‐3) for the Mars Express mission. Space Science Reviews, 126, 113 – 164. | |
dc.identifier.citedreference | Barabash, S., Fedorov, A., Lundin, R., & Sauvaud, J.‐A. ( 2007 ). Martian atmospheric erosion rates. Science, 315 ( 5811 ), 501 – 503. https://doi.org/10.1126/science.1134358 | |
dc.identifier.citedreference | Boesswetter, A., Bagdonat, T., Motschmann, U., & Sauer, K. ( 2004 ). Plasma boundaries at Mars: A 3‐D simulation study. Annales de Geophysique, 22 ( 12 ), 4363 – 4379. https://doi.org/10.5194/angeo‐22‐4363‐2004 | |
dc.identifier.citedreference | Brain, D. A., Halekas, J. S., Lillis, R., Mitchell, D. L., Lin, R. P., & Crider, D. H. ( 2005 ). Variability of the altitude of the Martian sheath. Geophysical Research Letters, 32, L18203. https://doi.org/10.1029/2005GL023126 | |
dc.identifier.citedreference | Brain, D. A., Mitchell, D. L., & Halekas, J. S. ( 2006 ). The magnetic field draping direction at Mars from April 1999 through August 2004. Icarus, 182 ( 2 ), 464 – 473. https://doi.org/10.1016/j.icarus.2005.09.023 | |
dc.identifier.citedreference | Brain, D. A., McFadden, J. P., Halekas, J. S., Connerney, J. E. P., Bougher, S. W., Curry, S., … Seki, K. ( 2015 ). The spatial distribution of planetary ion fluxes near Mars observed by MAVEN. Geophysical Research Letters, 42, 9142 – 9148. https://doi.org/10.1002/2015GL065293 | |
dc.identifier.citedreference | Carlsson, E., Brain, D., Luhmann, J., Barabash, S., Grigoriev, A., Nilsson, H., & Lundin, R. ( 2008 ). Influence of IMF draping direction and crustal magnetic field location on Martian ion beams. Planetary and Space Science, 56 ( 6 ), 861 – 867. https://doi.org/10.1016/j.pss.2007.12.016 | |
dc.identifier.citedreference | Curry, S. M., Liemohn, M. W., Fang, X., Ma, Y., Nagy, A. F., & Espley, J. ( 2013 ). The influence of production mechanisms on pickup ion loss at Mars. Journal of Geophysical Research: Space Physics, 118, 554 – 569. https://doi.org/10.1029/2012JA017665 | |
dc.identifier.citedreference | Dieval, C., Morgan, D. D., Nemec, F., & Gurnett, D. A. ( 2014 ). MARSIS observations of the Martian nightside ionosphere dependence on solar wind conditions. Journal of Geophysical Research: Space Physics, 119, 4077 – 4093. https://doi.org/10.1002/2014JA019788 | |
dc.identifier.citedreference | Dong, Y., Fang, X., Brain, D. A., McFadden, J. P., Halekas, J. S., Connerney, J. E., … Jakosky, B. M. ( 2015 ). Strong plume fl uxes at Mars observed by MAVEN: An important planetary ion escape channel. Geophysical Research Letters, 42, 8942 – 8950. https://doi.org/10.1002/2015GL065346 | |
dc.identifier.citedreference | Dong, Y., Fang, X., Brain, D. A., McFadden, J. P., Halekas, J. S., Connerney, J. E. P., … Jakosky, B. M. ( 2017 ). Seasonal variability of Martian ion escape through the plume and tail from MAVEN observations. Journal of Geophysical Research: Space Physics, 122, 4009 – 4022. https://doi.org/10.1002/2016JA023517 | |
dc.identifier.citedreference | Dubinin, E. M., Sauer, K., Lundin, R., Baumgärtel, K., & Bogdanov, A. ( 1996 ). Structuring of the transition region (plasma mantle) of the Martian magnetosphere. Geophysical Research Letters, 23 ( 7 ), 785 – 788. | |
dc.identifier.citedreference | Dubinin, E., Fränz, M., Woch, J., Roussos, E., Barabash, S., Lundin, R., … Acuña, M. ( 2006 ). Plasma morphology at Mars. Aspera‐3 observations. Space Science Reviews, 126 ( 1‐4 ), 209 – 238. https://doi.org/10.1007/s11214‐006‐9039‐4 | |
dc.identifier.citedreference | Dubinin, E., Fränz, M., Woch, J., Roussos, E., Barabash, S., Lundin, R., … Acuña, M. ( 2008 ). Plasma morphology at Mars: ASPERA‐3 observations. Space Science Reviews, 126 ( 1‐4 ), 209 – 238. https://doi.org/10.1007/s11214‐006‐9039‐4 | |
dc.identifier.citedreference | Dubinin, E., Fraenz, M., Fedorov, A., Lundin, R., Edberg, N., Duru, F., & Vaisberg, O. ( 2011 ). Ion energization and escape on Mars and Venus. Space Science Reviews, 162 ( 1‐4 ), 173 – 211. https://doi.org/10.1007/s11214‐011‐9831‐7 | |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
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