The substructure of a flux transfer event observed by the MMS spacecraft. Issue 18 (23rd September 2016)

• Record Type: Journal Article
• Authors: Hwang, K.‐J.; Sibeck, D. G.; Giles, B. L.; Pollock, C. J.; Gershman, D.; Avanov, L.; Paterson, W. R.; Dorelli, J. C.; Ergun, R. E.; Russell, C. T.; Strangeway, R. J.; Mauk, B.; Cohen, I. J.; Torbert, R. B.; Burch, J. L.
• Is Part Of: Geophysical research letters. Volume 43:Issue 18(2016)
• Page Start: 9434
• Page End: 9443
• Publication Date: 2016-09-23
• Subjects: flux transfer event -- FTE -- MMS -- reconnection -- flux rope -- magnetopause; Geophysics -- Periodicals; Planets -- Periodicals; Lunar geology -- Periodicals; 550
• DOI: 10.1002/2016GL070934
• Languages: English
• ISSNs: 0094-8276

Abstract

Abstract: On 15 August 2015, MMS (Magnetospheric Multiscale mission), skimming the dusk magnetopause, detected an isolated region of an increased magnetic strength and bipolar Bn, indicating a flux transfer event (FTE). The four spacecraft in a tetrahedron allowed for investigations of the shape and motion of the FTE. In particular, high‐resolution particle data facilitated our exploration of FTE substructures and their magnetic connectivity inside and surrounding the FTE. Combined field and plasma observations suggest that the core fields are open, magnetically connected to the northern magnetosphere from which high‐energy particles leak; ion "D" distributions characterize the axis of flux ropes that carry old‐opened field lines; counterstreaming electrons superposed by parallel‐heated components populate the periphery surrounding the FTE; and the interface between the core and draped regions contains a separatrix of newly opened magnetic field lines that emanate from the X line above the FTE. Key Points: Multilayers of open and draped fields in and around the FTE exhibit rapid‐varying connectivities to the magnetosphere and the FTE The interface between the core and draped regions contains a separatrix of newly opened magnetic field lines D‐shaped ion distributions feature the axis of flux ropes that carry old‐opened field lines