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|Title:||Magnetosonic Mach number dependence of the efficiency of reconnection between planetary and interplanetary magnetic fields|
Badman, S. V.
Cowley, S. W. H.
Milan, Steve E.
Nichols, Jonathan D.
Yeoman, Tim K.
|Publisher:||American Geophysical Union (AGU)|
|Citation:||Journal of Geophysical Research: Space Physics, 2009, 114, A07219.|
|Abstract:||We present a statistical investigation into the magnetosonic Mach number dependence of the efficiency of reconnection at the Earth's dayside magnetopause. We use the transpolar voltage V PC, derived from radar observations of the ionospheric electric field, as a proxy for the dayside reconnection voltage. Our results show that the IMF clock angle dependence of V PC is closely approximated by the function f() = sin2(/2), which we use in the derivation of a solar wind transfer function E* = E SW f(), wherein E SW is the solar wind electric field. We find that V PC is strongly related to E*, increasing almost linearly with small E* but saturating as E* becomes high. We also find that E* is strongly dependent on the magnetosonic Mach number, M MS, decreasing to near-zero values as M MS approaches 12, due principally to decreasing values of the IMF strength. V PC, on the other hand, is only weakly related to M MS and, for lower, more usual values of E*, actually shows a modest increase with increasing M MS. This result has implications for the solar wind-magnetosphere interaction at the outer planets where the Mach number is typically much higher than it is at 1 AU. Examples of SuperDARN convection maps from two high Mach number intervals are also presented, illustrating the existence of fairly typical reconnection driven flows. We thus find no evidence for a significant reduction in the magnetopause reconnection rate associated with high magnetosonic Mach numbers.|
|Rights:||This paper was published as Journal of Geophysical Research: Space Physics, 2009, 114, A07219. It is also available from http://www.agu.org/pubs/crossref/2009/2009JA014330.shtml. Doi: 10.1029/2009JA014330 To view the published open abstract, go to http://dx.doi.org and enter the DOI.|
|Appears in Collections:||Published Articles, Dept. of Physics and Astronomy|
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