Work

Observations and Simulations of a Double‐Core Hot Flow Anomaly

Year: 2024

Type: article

Abstract: Hot Flow anomalies (HFAs), one of the most well‐analyzed transient phenomena in the Earth's foreshock, are known as kinetic structures driven by tangential discontinuities (TDs). Recently, a 2‐dimensional (2D) magnetohydrodynamics (MHD) model reproduced HFAs with either a high‐ or low‐density core. Further investigation of an HFA with two cores observed by the Magnetospheric Multiscale (MMS) mission is reported. The observation via the Acceleration, Reconnection, Turbulence and Electrodynamics of the Moon's Interaction with the Sun (ARTEMIS) mission suggests this MHD HFA is associated with a foreshock density hole‐like structure. The trailing flux tube in simulation may propagate with a TD in the foreshock. Our work suggests that HFAs with two low‐density cores can also be achieved in MHD process. Results show the total ram pressure can be an excellent diagnostic for the presence of transient structures, such as HFAs, at the bow shock.

Source: Geophysical Research Letters

DOI: 10.1029/2024gl110363

Authors: Xi Lu, Antonius Otto, Hui Zhang, Terry Liu, Xingran Chen

Institutions: University of Alaska Fairbanks, University of California, Los Angeles

Language: English

Topic: Ionosphere and magnetosphere dynamics

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: gold

Estimated APC paid: $2,900

Funders: National Aeronautics and Space Administration, Nuclear Safety and Security Commission, Heliophysics Division