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The polar cusp location and its dependence on dipole tilt
Author(s) -
Zhou X.W.,
Russell C. T.,
Le G.,
Fuselier S. A.,
Scudder J. D.
Publication year - 1999
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 - 10.1029/1998gl900312
Subject(s) - cusp (singularity) , polar , magnetosheath , physics , magnetopause , field line , dipole , magnetosphere , tilt (camera) , geodesy , latitude , dipole model of the earth's magnetic field , geophysics , astrophysics , magnetic field , geometry , interplanetary magnetic field , solar wind , geology , astronomy , mathematics , quantum mechanics
Polar cusp crossings at high altitudes are seen in the POLAR data as decreases in the magnetic field and increases in magnetosheath‐like plasma. Close to 500 polar cusp crossings identified from the magnetic field, low‐energy electron and ion data observed by POLAR, are used to determine the statistical location of the polar cusp. When compared with Tsyganenko's 1989 vacuum model with an ellipsoidal magnetopause [ Tsyganenko , 1989], the medians of the cusp crossings are located between the magnetic field lines with invariant latitudes of 80° and 82°. Statistically the shape of the polar cusp in this region is consistent with this model although there is much scatter around the median value. The position of the cusp is significantly dependent on the dipole tilt angle. When dipole tilts more toward the Sun, the cusp moves more poleward to higher invariant latitude from 77.2° at −30° tilt, to 80.0° at 0° tilt, to 81.8° at 30° or roughly 1° for every 14° of tilt.