Europlanet Science Congress 2020
Virtual meeting
21 September – 9 October 2020
Europlanet Science Congress 2020
Virtual meeting
21 September – 9 October 2020
EPSC Abstracts
Vol.14, EPSC2020-985, 2020
https://doi.org/10.5194/epsc2020-985
Europlanet Science Congress 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

The fine structure of the subsolar MPB current layer from MAVEN observations: Implications for the Lorentz force

Gabriela Boscoboinik1,2, Cesar Bertucci1,2, Daniel Gomez1,2, Laura Morales2,3, Christian Mazelle4, Leonardo Regoli5, Jasper Halekas6, Jacob Gruesbeck7, David Mitchell8, and Bruce Jakosky9
Gabriela Boscoboinik et al.
  • 1Institute for Astronomy and Space Physics (IAFE), Buenos Aires, Argentina (cbertucci@iafe.uba.ar)
  • 2Departament of Physics, FCEyN, UBA, Buenos Aires, Argentina
  • 3INFIP, UBA/CONICET, Buenos Aires, Argentina
  • 4IRAP, UPS CNRS CNES, Toulouse, France
  • 5The Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland, USA
  • 6University of Iowa, Iowa City, IA, USA
  • 7GSFC, Greenbelt, MD, USA
  • 8SSL, University of California, Berkeley, USA
  • 9LASP, University of Colorado, Boulder, CO, USA

We report on the local structure of the Martian subsolar Magnetic Pileup Boundary (MPB) from minimum variance analysis of the magnetic field measured by the MAVEN spacecraft for six orbits. In particular, we detect a well defined current layer within the MPB’s fine structure and
provide a local estimate of its current density and compare these results with the current density obtained by multi-fluid simulations.
This current is of the order of hundreds of nAm-2 which results in a sunward Lorentz force of the order of 10-14 Nm-3. We compare these results with multifluid numerical simulations.
This force is associated with the gradient of the magnetic pressure, it accounts for the deflection of the solar wind ions near the MPB and for the acceleration of solar wind electrons which carry the interplanetary magnetic field through the MPB into the MPR. We also find that the
thickness of the MPB current layer is of the order of both the upstream (magnetosheath) solar wind proton inertial length and convective gyroradius. The former is consistent with the demagnetization of the ions due to the Hall electric field, an effect observed recently at the Earth magnetopause, while the latter would imply kinetic processes are important at the MPB.
This study supports recent results that report the presence of a steady current system around Mars in a similar way to the Earth.

How to cite: Boscoboinik, G., Bertucci, C., Gomez, D., Morales, L., Mazelle, C., Regoli, L., Halekas, J., Gruesbeck, J., Mitchell, D., and Jakosky, B.: The fine structure of the subsolar MPB current layer from MAVEN observations: Implications for the Lorentz force, Europlanet Science Congress 2020, online, 21 September–9 Oct 2020, EPSC2020-985, https://doi.org/10.5194/epsc2020-985, 2020