We present, for the first time, observational evidence of a kinetic electric field near the X-line associated with asymmetric reconnection at the Earth's dayside magnetopause using Polar observations. On March 29, 2003, Polar satellite detected an asymmetric collisionless reconnection event. This event shows a unipolar Hall electric field signature and a simple deviation from the guide field during the magnetopause crossing, with the absence of an ion plasma jet outflow indicating that the magnetopause crossing was near the X-line. As expected from particle-in-cell simulations by Malakit et al. (Phys. Rev. Lett. 111, 135001 (2013)), an earthward pointing normal electric field appears in the magnetospheric side of the ion diffusion region. The electric field satisfies two necessary conditions for the existence of the finite ion Larmor radius effect: (1) the ion Larmor radius (r(g2)) is larger than the distance between the stagnation point and the edge of the ion diffusion region in the strong magnetic field side (delta(S2)) and (2) the spatial extent of the kinetic electric field (delta(EL)) is of the order of the ion Larmor radius. Furthermore, it is shown that the peak value of the Larmor electric field is comparable to the predicted value. The observation of the Larmor electric field can be valuable in other analyses to show that the crossing occurred near the X-line. (C) 2014 AIP Publishing LLC.
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Shandong Institute of Advanced Technology, Jinan, ChinaShandong Institute of Advanced Technology, Jinan, China
Song, Xiaojian
Zuo, Pingbing
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Laboratory for Space Weather Storms, Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, ChinaShandong Institute of Advanced Technology, Jinan, China
Zuo, Pingbing
Shen, Zhenning
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Laboratory for Space Weather Storms, Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, ChinaShandong Institute of Advanced Technology, Jinan, China
Shen, Zhenning
Feng, Xueshang
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Laboratory for Space Weather Storms, Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, ChinaShandong Institute of Advanced Technology, Jinan, China
Feng, Xueshang
Xu, Xiaojun
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State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, ChinaShandong Institute of Advanced Technology, Jinan, China
Xu, Xiaojun
Wang, Yi
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Laboratory for Space Weather Storms, Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, ChinaShandong Institute of Advanced Technology, Jinan, China
Wang, Yi
Jiang, Chaowei
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Laboratory for Space Weather Storms, Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, ChinaShandong Institute of Advanced Technology, Jinan, China
Jiang, Chaowei
Luo, Xi
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Shandong Institute of Advanced Technology, Jinan, ChinaShandong Institute of Advanced Technology, Jinan, China
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Univ Texas San Antonio, Dept Phys & Astron, San Antonio, TX 78249 USA
Southwest Res Inst, San Antonio, TX 78238 USAUniv Texas San Antonio, Dept Phys & Astron, San Antonio, TX 78249 USA
Pritchard, K. R.
Burch, J. L.
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Southwest Res Inst, San Antonio, TX 78238 USAUniv Texas San Antonio, Dept Phys & Astron, San Antonio, TX 78249 USA
Burch, J. L.
Fuselier, S. A.
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Univ Texas San Antonio, Dept Phys & Astron, San Antonio, TX 78249 USA
Southwest Res Inst, San Antonio, TX 78238 USAUniv Texas San Antonio, Dept Phys & Astron, San Antonio, TX 78249 USA
Fuselier, S. A.
Genestreti, K. J.
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Southwest Res Inst, Durham, NH USAUniv Texas San Antonio, Dept Phys & Astron, San Antonio, TX 78249 USA
Genestreti, K. J.
Denton, R. E.
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Dartmouth Coll, Hanover, NH USAUniv Texas San Antonio, Dept Phys & Astron, San Antonio, TX 78249 USA
Denton, R. E.
Webster, J. M.
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Rice Univ, Houston, TX USAUniv Texas San Antonio, Dept Phys & Astron, San Antonio, TX 78249 USA
Webster, J. M.
Broll, J. M.
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Los Alamos Natl Lab, Los Alamos, NM USAUniv Texas San Antonio, Dept Phys & Astron, San Antonio, TX 78249 USA