EarthRef.org Reference Database (ERR)
Development and Maintenance by the EarthRef.org Database Team

Detailed Reference Information
Farrugia et al. 2000
Farrugia, C.J., Singer, H.J., Evans, D., Berdichevsky, D., Scudder, J.D., Ogilvie, K.W., Fitzenreiter, R.J. and Russell, C.T. (2000). Response of the equatorial and polar magnetosphere to the very tenuous solar wind on May 11, 1999. Geophysical Research Letters 27: doi: 10.1029/2000GL003800. issn: 0094-8276.

We examine effects in the equatorial and polar magnetosphere during 9--13 May, 1999. Earth's field at geostationary orbit became closely dipolar for ~16 hours when solar wind densities nsw were <1 cm-3. Electron precipitation in the northern polar cap intensified as nsw decreased, with significant fluxes up to ~15 keV energy on May 11. The simultaneous precipitation void in the southern polar cap implies a very pronounced north-south asymmetry, also reflected in the hemispherical power deposition. With an intense and collimated strahl, these observations support the ideas of Fairfield and Scudder [1985> on the preferential entry of the strahl into the northern hemisphere under the observed IMF away sector as a source of the north-south precipitation asymmetry. The polar rain north-south asymmetry argues against an ejecta source for the solar wind drop-out. The temporal profiles of solar wind parameters were very asymmetric with respect to the time of minimum nsw, and strong compressions and substorm activity prevailed as nsw recovered. ¿ 2000 American Geophysical Union

BACKGROUND DATA FILES

Abstract

Keywords
Interplanetary Physics, Solar wind plasma, Ionosphere, Particle precipitation, Ionosphere, Polar cap ionosphere, Magnetospheric Physics, Magnetospheric configuration and dynamics
Journal
Geophysical Research Letters
http://www.agu.org/journals/gl/
Publisher
American Geophysical Union
2000 Florida Avenue N.W.
Washington, D.C. 20009-1277
USA
1-202-462-6900
1-202-328-0566
service@agu.org
Click to clear formClick to return to previous pageClick to submit