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The substructure of a flux transfer event observed by the MMS spacecraft
Author(s) -
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.
Publication year - 2016
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1002/2016gl070934
Subject(s) - spacecraft , physics , magnetopause , magnetosphere , field line , flux (metallurgy) , magnetic field , event (particle physics) , magnetic flux , geophysics , plasma , magnetosheath , computational physics , astrophysics , astronomy , nuclear physics , materials science , quantum mechanics , metallurgy
On 15 August 2015, MMS (Magnetospheric Multiscale mission), skimming the dusk magnetopause, detected an isolated region of an increased magnetic strength and bipolar B n , 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.