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Observations of Mercury’s Bow Shock Disappearance in Quiet Solar Wind

  • Authors: Peishan He, Xiaojun Xu, Qing Chang

Peishan He et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 1.

Time-series observations of the solar wind interaction with Mercury’s magnetosphere on 2011 December 26. Panels give the magnitude of the magnetic field ∣B∣, the three components (BX, BY and BZ) of the magnetic field in the MSO coordinate system, respectively, and display the solar zenith angle. The arrows mark the identified boundaries of the bow shock (in yellow) and the magnetopause (in blue).

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