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A Double Disturbed Lunar Plasma Wake

Rasca, A.P. (author)
NASA Goddard Space Flight Center, MD, Greenbelt, United States
Fatemi, Shahab (author)
Umeå universitet,Institutionen för fysik
Farrell, W.M. (author)
NASA Goddard Space Flight Center, MD, Greenbelt, United States
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Poppe, A.R. (author)
Space Sciences Laboratory, University of California, CA, Berkeley, United States; Solar System Exploration Research Virtual Institute, NASA Ames Research Center, CA, Moffett Field, United States
Zheng, Y. (author)
NASA Goddard Space Flight Center, MD, Greenbelt, United States
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 (creator_code:org_t)
AGU, 2021
2021
English.
In: Journal of Geophysical Research - Space Physics. - : AGU. - 2169-9380 .- 2169-9402. ; 126:2
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • Under nominal solar wind conditions, a tenuous wake forms downstream of the lunar nightside. However, the lunar plasma environment undergoes a transformation as the Moon passes through the Earth's magnetotail, with hot subsonic plasma causing the wake structure to disappear. We investigate the lunar wake response during a passing coronal mass ejection (CME) on March 8, 2012 while crossing the Earth's magnetotail using both a magnetohydrodynamic (MHD) model of the terrestrial magnetosphere and a three-dimensional hybrid plasma model of the lunar wake. The CME arrives at 1 AU around 10:30 UT and its impact is first detected inside the geomagnetic tail after 11:10 UT by the Acceleration, Reconnection, Turbulence and Electrodynamics of the Moon's Interaction with the Sun (THEMIS-ARTEMIS) satellites in lunar orbit. A global magnetospheric MHD simulation using Wind data for upstream conditions with the OpenGGCM model reveals the magnetosheath compression to the lunar position from 11:20–12:00 UT, accompanied by multiple flux rope or plasmoid-like features developing and propagating tailward. MHD results support plasma changes observed by the THEMIS-ARTEMIS satellites. Lunar-scale simulations using the Amitis hybrid code show a short and misaligned plasma wake during the Moon's brief entry into the magnetosheath at 11:20 UT, with plasma expansion into the void being aided by the higher plasma temperatures. Sharply accelerated flow speed and a compressed magnetic field lead to an enhanced electric field in the lunar wake capable of generating sudden changes to the nightside near-surface electric potential.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Fusion, plasma och rymdfysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Fusion, Plasma and Space Physics (hsv//eng)

Keyword

hybrid simulation
Lunar wake
magnetotail
plasma
solar storm

Publication and Content Type

ref (subject category)
art (subject category)

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By the author/editor
Rasca, A.P.
Fatemi, Shahab
Farrell, W.M.
Poppe, A.R.
Zheng, Y.
About the subject
NATURAL SCIENCES
NATURAL SCIENCES
and Physical Science ...
and Astronomy Astrop ...
NATURAL SCIENCES
NATURAL SCIENCES
and Physical Science ...
and Fusion Plasma an ...
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Journal of Geoph ...
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Umeå University

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