Open AccessCusp observations of high‐ and low‐latitude reconnection for northward IMF: An alternate view
Author(s) -
Russell C. T.,
Le G.,
Petrinec S. M.
Publication year - 2000
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/1999ja900489
Subject(s) - magnetosheath , magnetosphere , magnetopause , interplanetary magnetic field , geophysics , solar wind , physics , cusp (singularity) , magnetic reconnection , polar , earth's magnetic field , field line , astrophysics , magnetic field , astronomy , geometry , mathematics , quantum mechanics
During high solar wind dynamic pressure, northward interplanetary magnetic field (IMF) intervals, the POLAR/TIMAS instrument observes angular distribution functions, that have been interpreted in terms of reconnection, below the latitude of the cusp, of nearly parallel magnetic field lines from the magnetosheath with those in the magnetosphere. If true, this process would lead to erosion of the dayside magnetosphere by northward IMF, a process not consistent with the observed control by IMF B z of the location of the dayside magnetopause, of the polar cusp, or of geomagnetic activity. However, we note that the TIMAS observations do not require such an interpretation and that a simpler interpretation exists, consistent with the current paradigm of IMF effects on the magnetosphere.