Four-sheet structures of dayside field-aligned currents: Statistical study

Details Four-sheet structures of dayside field-aligned currents: Statistical study Four-sheet structures of dayside field-aligned currents: Statistical study

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000jgr...10525317o&link_type=abstract

Journal of Geophysical Research, Volume 105, Issue A11, p. 25317-25324

Physics

10

Magnetospheric Physics

Scientific paper

The present study investigates the statistical characteristics of four-sheet structures of large-scale field-aligned currents (FACs) observed by the Defense Meteorological Satellite Program-F7 (DMSP-F7) satellite in the dayside high-latitude region. A total of 495 four-FAC-sheet events were selected from the entire set of DMSP-F7 magnetometer data. With respect to the polarity of FACs, the selected events are classified into two groups, which are named type M and type W after the shape of a plot of the azimuthal magnetic component. The polarity of the equatorward most FAC is downward for the type M structure, whereas it is upward for the type W structure. Type W and type M events tend to take place in the prenoon and postnoon sectors, respectively, but the transition takes place slightly before noon. The type W structure tends to be observed for negative and positive interplanetary magnetic field (IMF) BY in the Northern and Southern Hemispheres, respectively. For a given hemisphere, the favorable sign of IMF BY for the type M structure is opposite to that for the type W structure. It is also found that both types occur more often when the IMF BZ is northward than when it is southward. The four-sheet structure can be interpreted in terms of two zonal ionospheric convection flows separated in latitude. The equatorward one is a part of the viscous cell and, possibly, also the merging cell, whereas the poleward one is a part of the lobe cell. The direction (of the major cell) of the lobe convection is determined by the sign of IMF BY and is different in different hemispheres, explaining the discovered IMF BY dependence. The preference for northward IMF BZ is consistent with the required development of the lobe convection. It is inferred from the expected polar distribution of FACs that the four-sheet structure is a superposition of a pair of midday region 0 and region 1 currents and a pair of conventional region 1 and region 2 currents.

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