Physics
Scientific paper
May 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agusmsm51a..02n&link_type=abstract
American Geophysical Union, Spring Meeting 2007, abstract #SM51A-02
Physics
2431 Ionosphere/Magnetosphere Interactions (2736), 2716 Energetic Particles: Precipitating, 2724 Magnetopause And Boundary Layers, 2784 Solar Wind/Magnetosphere Interactions
Scientific paper
The traditional distinction between a northward and southward IMF cusp is deficient, in that northward IMF cusp encounters often closely resemble southward IMF encounters. Partly for that reason, "southward" IMF cusps have been far more often examined than "northward." Recently Newell et al. [2007] showed that the magnetopause merging rate, dFMP/dt, much better predicts cusp latitude than does Bz (or Bs). Here, we investigate the extent to which high and low merging rate conditions better separate cusp encounters into mutually distinct classes. Indeed, high merging rate cusps (those with dFMP/dt > 2*
Newell Patrick T.
Rich Frederic J.
Wing Simon
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