The Twisted Configuration of the Martian Magnetotail: MAVEN Observations

Measurements provided by the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft are analyzed to investigate the Martian magnetotail configuration as a function of interplanetary magnetic field (IMF) BY. We find that the magnetotail lobes exhibit a ~45deg twist, either clockwise or countercloc...

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Vydané v:	Geophysical research letters Ročník 45; číslo 10; s. 4559 - 4568
Hlavní autori:	DiBraccio, Gina A., Luhmann, Janet G., Curry, Shannon M., Espley, Jared R., Xu, Shaosui, Mitchell, David L., Ma, Yingjuan, Dong, Chuanfei, Gruesbeck, Jacob R., Connerney, John E. P., Harada, Yuki, Ruhunusiri, Suranga, Halekas, Jasper S., Soobiah, Yasir, Hara, Takuya, Brain, David A., Jakosky, Bruce M.
Médium:	Journal Article
Jazyk:	English
Vydavateľské údaje:	Goddard Space Flight Center American Geophysical Union 28.05.2018 John Wiley & Sons, Inc
Predmet:	Aerosols Atmospheric evolution Computational fluid dynamics Computer simulation Configurations Earth Fluid flow Geometry Interplanetary magnetic field Investigations Lobes Lunar And Planetary Science And Exploration Magnetic field magnetic field topology Magnetic fields Magnetic reconnection Magnetohydrodynamic simulation Magnetotails Mars Mars atmosphere Mars crustal magnetic fields Mars environment Mars magnetotail configuration Mars missions Mars spacecraft MAVEN data Planetary magnetic fields Planets Rotation solar wind‐Mars interaction Spacecraft Venus Configuration Magnetotail Martian
ISSN:	0094-8276, 1944-8007
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Abstract	Measurements provided by the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft are analyzed to investigate the Martian magnetotail configuration as a function of interplanetary magnetic field (IMF) BY. We find that the magnetotail lobes exhibit a ~45deg twist, either clockwise or counterclockwise from the ecliptic plane, up to a few Mars radii downstream. Moreover, the associated cross-tail current sheet is rotated away from the expected location for a Venus-like induced magnetotail based on nominal IMF draping. Data-model comparisons using magnetohydrodynamic simulations are in good agreement with the observed tail twist. Model field line tracings indicate that a majority of the twisted tail lobes are composed of open field lines, surrounded by draped IMF. We infer that dayside magnetic reconnection between the crustal fields and draped IMF creates these open fields and may be responsible for the twisted tail configuration, similar to what is observed at Earth.
AbstractList	Measurements provided by the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft are analyzed to investigate the Martian magnetotail configuration as a function of interplanetary magnetic field (IMF) BY. We find that the magnetotail lobes exhibit a ~45° twist, either clockwise or counterclockwise from the ecliptic plane, up to a few Mars radii downstream. Moreover, the associated cross‐tail current sheet is rotated away from the expected location for a Venus‐like induced magnetotail based on nominal IMF draping. Data‐model comparisons using magnetohydrodynamic simulations are in good agreement with the observed tail twist. Model field line tracings indicate that a majority of the twisted tail lobes are composed of open field lines, surrounded by draped IMF. We infer that dayside magnetic reconnection between the crustal fields and draped IMF creates these open fields and may be responsible for the twisted tail configuration, similar to what is observed at Earth. Plain Language Summary This study investigates the magnetic environment of Mars in order to understand how its structure is different from that of other planets. In the past, it was thought that the Sun's magnetic field interacts with Mars in a similar way to a comet or Venus. This would imply that the magnetic field geometry could be easily predicted; however, recent investigations have found that this is not the case. This work includes both simulation and MAVEN data to determine that the magnetic environment of Mars is much different than this original picture. The conclusions find that these fields are twisted from their expected geometry, suggesting a difference in the interaction between Mars and the Sun. Because atmospheric particles are able to travel along these magnetic fields, this unique geometry may have great implications for atmospheric loss at Mars. Key Points MAVEN data and simulations confirm that a twisted field configuration is present in the Martian magnetotail that is highly dependent on IMF BY Open fields, likely created by magnetic reconnection between Mars crustal fields and the IMF, occupy a majority of the twisted tail lobes Comparisons with Earth suggest that the dipolar component of Mars' crustal fields play a crucial role in altering the magnetotail structure Measurements provided by the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft are analyzed to investigate the Martian magnetotail configuration as a function of interplanetary magnetic field (IMF) B Y . We find that the magnetotail lobes exhibit a ~45° twist, either clockwise or counterclockwise from the ecliptic plane, up to a few Mars radii downstream. Moreover, the associated cross‐tail current sheet is rotated away from the expected location for a Venus‐like induced magnetotail based on nominal IMF draping. Data‐model comparisons using magnetohydrodynamic simulations are in good agreement with the observed tail twist. Model field line tracings indicate that a majority of the twisted tail lobes are composed of open field lines, surrounded by draped IMF. We infer that dayside magnetic reconnection between the crustal fields and draped IMF creates these open fields and may be responsible for the twisted tail configuration, similar to what is observed at Earth. This study investigates the magnetic environment of Mars in order to understand how its structure is different from that of other planets. In the past, it was thought that the Sun's magnetic field interacts with Mars in a similar way to a comet or Venus. This would imply that the magnetic field geometry could be easily predicted; however, recent investigations have found that this is not the case. This work includes both simulation and MAVEN data to determine that the magnetic environment of Mars is much different than this original picture. The conclusions find that these fields are twisted from their expected geometry, suggesting a difference in the interaction between Mars and the Sun. Because atmospheric particles are able to travel along these magnetic fields, this unique geometry may have great implications for atmospheric loss at Mars. MAVEN data and simulations confirm that a twisted field configuration is present in the Martian magnetotail that is highly dependent on IMF B Y Open fields, likely created by magnetic reconnection between Mars crustal fields and the IMF, occupy a majority of the twisted tail lobes Comparisons with Earth suggest that the dipolar component of Mars' crustal fields play a crucial role in altering the magnetotail structure Measurements provided by the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft are analyzed to investigate the Martian magnetotail configuration as a function of interplanetary magnetic field (IMF) BY. We find that the magnetotail lobes exhibit a ~45deg twist, either clockwise or counterclockwise from the ecliptic plane, up to a few Mars radii downstream. Moreover, the associated cross-tail current sheet is rotated away from the expected location for a Venus-like induced magnetotail based on nominal IMF draping. Data-model comparisons using magnetohydrodynamic simulations are in good agreement with the observed tail twist. Model field line tracings indicate that a majority of the twisted tail lobes are composed of open field lines, surrounded by draped IMF. We infer that dayside magnetic reconnection between the crustal fields and draped IMF creates these open fields and may be responsible for the twisted tail configuration, similar to what is observed at Earth. Measurements provided by the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft are analyzed to investigate the Martian magnetotail configuration as a function of interplanetary magnetic field (IMF) BY. We find that the magnetotail lobes exhibit a ~45° twist, either clockwise or counterclockwise from the ecliptic plane, up to a few Mars radii downstream. Moreover, the associated cross‐tail current sheet is rotated away from the expected location for a Venus‐like induced magnetotail based on nominal IMF draping. Data‐model comparisons using magnetohydrodynamic simulations are in good agreement with the observed tail twist. Model field line tracings indicate that a majority of the twisted tail lobes are composed of open field lines, surrounded by draped IMF. We infer that dayside magnetic reconnection between the crustal fields and draped IMF creates these open fields and may be responsible for the twisted tail configuration, similar to what is observed at Earth.
Audience	PUBLIC
Author	Dong, Chuanfei Ma, Yingjuan Brain, David A. DiBraccio, Gina A. Harada, Yuki Gruesbeck, Jacob R. Hara, Takuya Mitchell, David L. Jakosky, Bruce M. Luhmann, Janet G. Soobiah, Yasir Xu, Shaosui Connerney, John E. P. Halekas, Jasper S. Espley, Jared R. Curry, Shannon M. Ruhunusiri, Suranga
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Snippet	Measurements provided by the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft are analyzed to investigate the Martian magnetotail configuration as a...
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SubjectTerms	Aerosols Atmospheric evolution Computational fluid dynamics Computer simulation Configurations Earth Fluid flow Geometry Interplanetary magnetic field Investigations Lobes Lunar And Planetary Science And Exploration Magnetic field magnetic field topology Magnetic fields Magnetic reconnection Magnetohydrodynamic simulation Magnetotails Mars Mars atmosphere Mars crustal magnetic fields Mars environment Mars magnetotail configuration Mars missions Mars spacecraft MAVEN data Planetary magnetic fields Planets Rotation solar wind‐Mars interaction Spacecraft Venus
Title	The Twisted Configuration of the Martian Magnetotail: MAVEN Observations
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