Articles | Volume 42, issue 1
https://doi.org/10.5194/angeo-42-79-2024
https://doi.org/10.5194/angeo-42-79-2024
Regular paper
 | 
07 Mar 2024
Regular paper |  | 07 Mar 2024

Scalar-potential mapping of the steady-state magnetosheath model

Yasuhito Narita, Daniel Schmid, and Simon Toepfer

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Cited articles

Angelopoulos, V. The THEMIS mission, Space Sci. Rev, 141, 5, https://doi.org/10.1007/s11214-008-9336-1, 2008. a
Cairns, I. H., Fairfield, D. H., Anderson, R. R., Carlton, V. E. H., Paularenas, K. I., and Lazarus, A.: Unusual locations of Earth's bow shock on September 24–25, 1987: Mach number effects, J. Geophys. Res., 100, 47–62, https://doi.org/10.1029/94JA01978, 1995. a, b, c
Chakravarthy, S. and Anderson, D.: Numerical conformal mapping, Math. Comp. 33, 953–969, 1979. a
Dimmock, A. P., and Nykyri, K: The statistical mapping of magnetosheath plasma properties based on THEMIS measurements in the magnetosheath interplanetary medium reference frame, J. Geophys. Res.-Space, 118, 4963–4976, https://doi.org/10.1002/jgra.50465, 2013. a
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The magnetosheath is a transition layer surrounding the planetary magnetosphere. We develop an algorithm to compute the plasma flow velocity and magnetic field for a more general shape of magnetosheath using the concept of potential field and suitable coordinate transformation. Application to the empirical Earth magnetosheath region is shown in the paper. The developed algorithm is useful when interpreting the spacecraft data or simulation of the planetary magnetosheath region.