 |
Detailed Reference Information |
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 |
|
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 |
|
|
 |