Magnetohydrodynamic Perspective on the Disappearance of Mercury’s Bow Shock by Helios Data Exploration

In the magnetohydrodynamic (MHD) perspective, the planet’s bow shock would disappear when the fast-mode Mach number ( M _F ) of the solar wind is less than one. Compared to Earth, Mercury is subject to a lower M _F solar wind due to its proximity to the Sun, resulting in a higher possibility of the...

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Bibliografiset tiedot

Päätekijät:	S. H. Lai, Y.-H. Yang, W.-H. Ip
Aineistotyyppi:	Artigo
Kieli:	Inglês
Julkaistu:	IOP Publishing 2024-01-01
Sarja:	The Astrophysical Journal
Aiheet:	Planetary bow shocks Mercury (planet) Solar wind Magnetohydrodynamics Solar cycle
Linkit:	https://doi.org/10.3847/1538-4357/ad0a8a
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