@Article{WangCSLRLGG:2024:DiDeOn,
author = "Wang, Rongsheng and Cheng, Zihang and Slavin, James A. and Lu,
Quanming and Raines, Jim and Lu, San and Guo, Jin and Gonzalez
Alarcon, Walter Demetrio",
affiliation = "{Deep Space Exploration Laboratory} and {University of Science and
Technology of China} and {University of Michigan} and {Deep Space
Exploration Laboratory} and {University of Michigan} and {Deep
Space Exploration Laboratory} and {University of Science and
Technology of China} and {Instituto Nacional de Pesquisas
Espaciais (INPE)}",
title = "Direct Detection of Ongoing Magnetic Reconnection at Mercury's
High-Latitude Magnetopause",
journal = "Geophysical Research Letters",
year = "2024",
volume = "51",
number = "5",
pages = "e2023GL106282",
month = "Mar.",
keywords = "Mercury's magnetosphere, magnetic reconnection, magnetic flux
ropes.",
abstract = "An ongoing magnetic reconnection event was detected in the
Mercury's high latitude magnetopause during a northward
interplanetary magnetic field. The reconnection X-line region was
revealed in the Mercury's magnetopause based on the encountered
flux ropes ejected away from this region both planetward and
tailward. A series of magnetic flux ropes, known as flux transfer
event shower were observed tailward of this X-line region. These
flux ropes were probably expanding and deflected as they were
ejected away tailward from the X-line region. Large-amplitude
variations in all three components of the magnetic field and a few
small-scale flux ropes were observed inside the X-line region,
which could be the seed of the flux rope shower at the
magnetopause. The observations suggest that magnetic reconnection
is highly dynamic and persistent in Mercury's magnetosphere.
Magnetic reconnection has been regarded as the most important
process for dynamics of the Mercury's magnetosphere and for the
interaction between the solar wind and the Mercury's magnetosphere
also. Although magnetic flux ropes and flux transfer events (FTEs)
resulting from magnetic reconnection have been extensively
observed in the Mercury's magnetosphere, the key region of
magnetic reconnection, namely the X-line region, has never been
reported so far by the spacecraft. Here, we present the first
evidence of the reconnection X-line region in the Mercury's
magnetosphere. A few small-scale magnetic flux ropes are observed
inside the reconnection X-line region, which could be the seed of
the observed magnetic FTE shower. Furthermore, the evolution of
these flux ropes is addressed also based on the spacecraft
observations. A reconnection X-line region is first observed in
the Mercury's magnetopause during the northward interplanetary
magnetic field The small-scale magnetic flux ropes in the X-line
region could be the seed of the flux transfer event shower The
flux ropes probably expand and is deflected after they are ejected
away from the X-line region.",
doi = "10.1029/2023GL106282",
url = "http://dx.doi.org/10.1029/2023GL106282",
issn = "0094-8276",
language = "en",
targetfile = "Geophysical Research Letters - 2024 - Wang - Direct Detection of
Ongoing Magnetic Reconnection at Mercury s
High\‐Latitude.pdf",
urlaccessdate = "29 jun. 2024"
}