Soft X-ray imaging of Earth's dayside magnetosheath and cusps using hybrid simulations

Abstract

Interactions between solar wind ions and neutral hydrogen atoms in Earth's exosphere can lead to the emission of soft X-rays. Upcoming missions such as SMILE and LEXI aim to use soft X-ray imaging to study the global structure of the magnetosphere. Although the magnetosheath and dayside magnetopause can often be driven by kinetic physics, it has typically been omitted from fluid simulations used to predict X-ray emissions. We study the possible results of soft X-ray imaging using hybrid simulations under quasi-radial interplanetary magnetic fields, where ion-ion instabilities drive ultra-low frequency foreshock waves, leading to turbulence in the magnetosheath, affecting the dynamics of the cusp and magnetopause. We simulate soft X-ray emission to determine what may be seen by missions such as LEXI, and evaluate the possibility of identifying kinetic structures. While kinetic structures are visible in high-cadence imaging, current instruments may not have the time resolution to discern kinetic signals.

References in corpus (5)

• Magnetopause expansions for quasi-radial interplanetary magnetic field: THEMIS and Geotail observations
• Identifying XMM-Newton observations affected by solar wind charge exchange - Part I
• AXIOM: Advanced X-ray Imaging Of the Magnetosphere
• Hybrid simulations of the cusp and dayside magnetosheath dynamics under \ quasi-radial interplanetary magnetic fields
• Soft X-Ray Imaging of Magnetopause Reconnection Outflows Under Low Plasma-$\beta$ Solar Wind Conditions