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Study of fluctuations in the Martian magnetosheath using a kurtosis technique:mars Express observations

Earth and Planetary Physics 2022年第1期6卷 28-41页

作者： A.M.S.Franco E.Echer M.J.A.Bolzan M.Fraenz National Institute for Space Research(INPE) Sao Jose dos CamposBrazil Federal University of Jatai JataiBrazil Max Planck Institute for Solar System Research GöttingenGermany

Planetary magnetosheaths are characterized by high plasma wave and turbulence *** Martian magnetosheath is no exception;both upstream and locally generated plasma waves have been observed in the region between its bow shock and magnetic boundary layer,its induced *** statistical study of wave activity in the Martian magnetosheath is based on 12 years(2005-2016)of observations made during mars Express(MEX)crossings of the planet’s magnetosheath-in particular,data on electron density and temperature data collected by the electron spectrometer(ELS)of the plasma analyzer(ASPERA-3)experiment on board the MEX spacecraft.A kurtosis parameter has been calculated for these plasma *** value indicates intermittent behavior in the data when it is higher than 3(the value for a normal or Gaussian distribution).The variation of wave activity occurrence has been analyzed in relation to solar cycle,Martian orbit,and distance to the bow ***-Gaussian properties are observed in the magnetosheath of mars on all analyzed scales,especially in those near the proton gyrofrequency in the upstream region of the Martian *** also report that non-Gaussian behavior is most prominent at the smaller scales(higher frequencies).A significant influence of the solar cycle was also observed;the kurtosis parameter is higher during declining and solar maximum phases,when the presence of disturbed solar wind conditions,caused by large scale solar wind structures,*** kurtosis decreases with increasing distance from the bow shock,which indicates that the intermittence level is higher near the bow *** the electron temperature data the kurtosis is higher near the perihelion due to the higher incidence of EUV when the planet is closer to the Sun,which causes a more extended exosphere,and consequently increases the wave activity in the magnetosheath and its upstream *** extended exosphere seems to play a lower effect in the electron den

关键词： mars magnetosheath kurtosis ULF waves

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