MMS observations of large guide field symmetric reconnection between colliding reconnection jets at the center of a magnetic flux rope at the magnetopause

M. ØierosetT. D. PhanC. HaggertyM. A. ShayJ. P. EastwoodD. J. GershmanJ. F. DrakeM. FujimotoR. E. ErgunF. S. MozerM. OkaR. B. TorbertJ. L. BurchS. WangL. J. ChenM. SwisdakC. PollockJ. C. DorelliS. A. FuselierB. LavraudB. L. GilesT. E. MooreY. SaitoL. A. AvanovW. PatersonR. J. StrangewayC. T. RussellY. KhotyaintsevP. A. LindqvistK. MalakitSpace Sciences Laboratory at UC BerkeleyUniversity of DelawareImperial College LondonNASA Goddard Space Flight CenterUniversity of MarylandJapan Aerospace Exploration AgencyUniversity of Colorado at BoulderUniversity System of New HampshireSouthwest Research InstituteDenali ScientificUniversity of Texas at San AntonioUniversite de ToulouseCNRS Centre National de la Recherche ScientifiqueUniversity of California, Los AngelesInstiutet för rymdfysikThe Royal Institute of Technology (KTH)Mahidol University2018-12-112019-03-142018-12-112019-03-142016-06-16Geophysical Research Letters. Vol.43, No.11 (2016), 5536-554419448007009482762-s2.0-84973157325https://repository.li.mahidol.ac.th/handle/20.500.14594/43555©2016. American Geophysical Union. All Rights Reserved. We report evidence for reconnection between colliding reconnection jets in a compressed current sheet at the center of a magnetic flux rope at Earth's magnetopause. The reconnection involved nearly symmetric inflow boundary conditions with a strong guide field of two. The thin (2.5 ion-skin depth (di) width) current sheet (at ~12 di downstream of the X line) was well resolved by MMS, which revealed large asymmetries in plasma and field structures in the exhaust. Ion perpendicular heating, electron parallel heating, and density compression occurred on one side of the exhaust, while ion parallel heating and density depression were shifted to the other side. The normal electric field and double out-of-plane (bifurcated) currents spanned almost the entire exhaust. These observations are in good agreement with a kinetic simulation for similar boundary conditions, demonstrating in new detail that the structure of large guide field symmetric reconnection is distinctly different from antiparallel reconnection.Mahidol UniversityEarth and Planetary SciencesMMS observations of large guide field symmetric reconnection between colliding reconnection jets at the center of a magnetic flux rope at the magnetopauseLetterSCOPUS10.1002/2016GL069166