Amplitude modulation of the equatorial electrojet (EEJ) during a magnetospheric storm

Details Amplitude modulation of the equatorial electrojet (EEJ) during a magnetospheric storm Amplitude modulation of the equatorial electrojet (EEJ) during a magnetospheric storm

Jul 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998jastp..60.1129s&link_type=abstract

Journal of Atmospheric and Solar-Terrestrial Physics, Volume 60, Issue 11, p. 1129-1137.

Physics

2

Scientific paper

An encounter of the Earth with a high velocity solar wind stream triggered the magnetic storm of 29 January 1995. The storm lasted for the following seven days, keeping the level of the Dst index in the range of -25--50 nT. At the dip-equator, a regular enhancement of the magnetic H component during daytime, referred to as the Equatorial Electrojet (EEJ), was seen to be suppressed and modified during this storm interval. We attempted to classify the type of the EEJ modification by analyzing magnetometer data from two stations at the dip-equator but located in the opposite hemisphere, and energetic particle data from two geosynchronous satellites located close to the ground magnetometer meridian. As a result, three different types of modulation of EEJ amplitudes, with time scales of 15 min to 1 day, were found to appear during the periods when the flux level of low energy charged particles (>30 keV) in the midnight magnetosphere was increased above the quiet level. These modulations were characterized by referring to the nightside particle signatures. We argue that, although the EEJ is a local enhancement of the ionospheric currents at the dayside dip-equator, the EEJ is definitely affected by changes of the magnetosphere, probably in various ways arising from the complexities of the storm effects.

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