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Reconnection at the dayside low‐latitude magnetopause and its nonrole in low‐latitude boundary layer formation during northward interplanetary magnetic field
Author(s) -
Phan TaiD.,
Oieroset Marit,
Fujimoto Masaki
Publication year - 2005
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 - 10.1029/2005gl023355
Subject(s) - magnetosheath , magnetopause , interplanetary magnetic field , physics , magnetic reconnection , geophysics , boundary layer , solar wind , cusp (singularity) , latitude , plasma sheet , magnetosphere , atmospheric sciences , astrophysics , plasma , mechanics , astronomy , geometry , mathematics , quantum mechanics
On 2001‐12‐02 Wind crossed the dayside magnetopause (MP) at ∼15 MLT and traversed the adjacent low‐latitude boundary layer (LLBL) over a period of 2 hours. The IMF was steady (northward and dawnward) during the MP/LLBL encounter. Reconnection flows were observed in the MP that were directed 130° away from the magnetosheath flow direction. In contrast, the LLBL flow was aligned with the magnetosheath flow. The counterstreaming field‐aligned and anti‐field‐aligned electrons have different energies and their fluxes are unbalanced in the open MP whereas they are precisely balanced throughout most of the LLBL indicative of a closed LLBL. These observations indicate that reconnection occurs at the low‐latitude MP during northward IMF (with a significant B y ), but low‐latitude reconnection is not responsible for the creation of the LLBL. Instead, reconnection appears to be in the process of eroding a pre‐existing LLBL that was created either by diffusive entry or by non‐simultaneous double‐cusp reconnection.