Articles | Volume 42, issue 1
https://doi.org/10.5194/angeo-42-117-2024
https://doi.org/10.5194/angeo-42-117-2024
Regular paper
 | 
25 Apr 2024
Regular paper |  | 25 Apr 2024

Short large-amplitude magnetic structures (SLAMS) at Mercury observed by MESSENGER

Tomas Karlsson, Ferdinand Plaschke, Austin N. Glass, and Jim M. Raines

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Cited articles

Anderson, B. J., Acuña, M. H., Lohr, D. A., Scheifele, J., Raval, A., Korth, H., and Slavin, J. A.: The Magnetometer instrument on MESSENGER, in: The MESSENGER mission to Mercury, Springer, 417–450, https://doi.org/10.1007/978-0-387-77214-1, 2007. a, b
Balogh, A. and Treumann, R. A.: Planetary Bow Shocks, in: Physics of Collisionless Shocks, Springer, 411–461, https://doi.org/10.1007/978-1-4614-6099-2, 2013. a
Bebesi, Z., Erdos, G., and Szego, K.: Observations of short large amplitude magnetic structures at the Kronian bow shock, Icarus, 333, 306–317, 2019. a, b
Behannon, K. W.: Heliocentric distance dependence of the interplanetary magnetic field, Rev. Geophys., 16, 125–145, 1978. a
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Short summary
The solar wind interacts with the planets in the solar system and creates a supersonic shock in front of them. The upstream region of this shock contains many complicated phenomena. One such phenomenon is small-scale structures of strong magnetic fields (SLAMS). These SLAMS have been observed at Earth and are important in determining the properties of space around the planet. Until now, SLAMS have not been observed at Mercury, but we show for the first time that SLAMS also exist there.
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