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Asymmetry in the Earth's magnetotail neutral sheet rotation due to IMF B-y sign?

Pitkänen, Timo, 1979- (author)
Umeå universitet,Institutionen för fysik,Shandong Provincial Key Laboratory of Optical Astronomy and Solar‑Terres‑ trial Environment, Institute of Space Sciences, Shandong University, Weihai, China; Space Physics and Astronomy Research Unit, University of Oulu, Oulu, Finland,Shandong Univ, Inst Space Sci, Shandong Prov Key Lab Opt Astron & Solar Terr Env, Weihai, Peoples R China.;Umeå Univ, Dept Phys, Umeå, Sweden.;Univ Oulu, Space Phys & Astron Res Unit, Oulu, Finland.
Kullen, Anita (author)
KTH,Rymd- och plasmafysik
Cai, Lei (author)
KTH,Rymd- och plasmafysik
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Park, Jong-Sun (author)
Shandong Univ, Inst Space Sci, Shandong Prov Key Lab Opt Astron & Solar Terr Env, Weihai, Peoples R China.
Vanhamaki, Heikki (author)
Univ Oulu, Space Phys & Astron Res Unit, Oulu, Finland.
Hamrin, Maria, 1972- (author)
Umeå universitet,Institutionen för fysik,Umeå Univ, Dept Phys, Umeå, Sweden.
Aikio, Anita T. (author)
Univ Oulu, Space Phys & Astron Res Unit, Oulu, Finland.
Chong, G. Siung (author)
Umeå universitet,Institutionen för fysik,Umeå Univ, Dept Phys, Umeå, Sweden.
De Spiegeleer, Alexandre (author)
Umeå universitet,Institutionen för fysik,Umeå Univ, Dept Phys, Umeå, Sweden.
Shi, Quanqi (author)
Shandong Univ, Inst Space Sci, Shandong Prov Key Lab Opt Astron & Solar Terr Env, Weihai, Peoples R China.
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 (creator_code:org_t)
2021-01-12
2021
English.
In: Geoscience Letters. - : Springer Nature. - 2196-4092. ; 8:1
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • Evidence suggests that a non-zero dawn-dusk interplanetary magnetic field (IMF B-y) can cause a rotation of the cross-tail current sheet/neutral sheet around its axis aligned with the Sun-Earth line in Earth's magnetotail. We use Geotail, THEMIS and Cluster data to statistically investigate how the rotation of the neutral sheet depends on the sign and magnitude of IMF B-y. In our dataset, we find that in the tail range of -30 < XGSM < -15 R-E, the degree of the neutral sheet rotation is clearly smaller, there appears no significant rotation or even, the rotation is clearly to an unexpected direction for negative IMF B-y, compared to positive IMF B-y. Comparison to a model by Tsyganenko et al. (2015, doi:10.5194/angeo-33-1-2015) suggests that this asymmetry in the neutral sheet rotation between positive and negative IMF B-y conditions is too large to be explained only by the currently known factors. The possible cause of the asymmetry remains unclear.

Subject headings

NATURVETENSKAP  -- Fysik -- Fusion, plasma och rymdfysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Fusion, Plasma and Space Physics (hsv//eng)

Keyword

Solar wind-magnetosphere interaction
Magnetosphere configuration
Magnetotail
Plasma sheet
Neutral sheet

Publication and Content Type

ref (subject category)
art (subject category)

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