<?xml version="1.0" encoding="UTF-8"?><xml><records><record><source-app name="Biblio" version="6.x">Drupal-Biblio</source-app><ref-type>17</ref-type><contributors><authors><author><style face="normal" font="default" size="100%">Don L. Carpenter</style></author><author><style face="normal" font="default" size="100%">Giles, B. L.</style></author><author><style face="normal" font="default" size="100%">Chappell, C. R.</style></author><author><style face="normal" font="default" size="100%">Décréau, P. M. E.</style></author><author><style face="normal" font="default" size="100%">Anderson, R. R.</style></author><author><style face="normal" font="default" size="100%">Persoon, A. M.</style></author><author><style face="normal" font="default" size="100%">Smith, A. J.</style></author><author><style face="normal" font="default" size="100%">Corcuff, Y.</style></author><author><style face="normal" font="default" size="100%">Canu, P.</style></author></authors></contributors><titles><title><style face="normal" font="default" size="100%">Plasmasphere dynamics in the duskside bulge region: A new look atold topic</style></title><secondary-title><style face="normal" font="default" size="100%">Journal of Geophysical Research</style></secondary-title></titles><keywords><keyword><style  face="normal" font="default" size="100%">BOUNDARY LAYER PLASMAS</style></keyword><keyword><style  face="normal" font="default" size="100%">CONVECTION</style></keyword><keyword><style  face="normal" font="default" size="100%">CONVECTIVE FLOW</style></keyword><keyword><style  face="normal" font="default" size="100%">DYNAMICS EXPLORER 1 SATELLITE</style></keyword><keyword><style  face="normal" font="default" size="100%">EROSION</style></keyword><keyword><style  face="normal" font="default" size="100%">GEOS 2 SATELLITE</style></keyword><keyword><style  face="normal" font="default" size="100%">INTERNATIONAL SUN EARTH EXPLORER 1</style></keyword><keyword><style  face="normal" font="default" size="100%">MAGNETIC STORMS</style></keyword><keyword><style  face="normal" font="default" size="100%">MAGNETOHYDRODYNAMIC STABILITY</style></keyword><keyword><style  face="normal" font="default" size="100%">MATHEMATICAL MODELS</style></keyword><keyword><style  face="normal" font="default" size="100%">PLASMA DRIFT</style></keyword><keyword><style  face="normal" font="default" size="100%">PLASMAPAUSE</style></keyword><keyword><style  face="normal" font="default" size="100%">plasmasphere</style></keyword><keyword><style  face="normal" font="default" size="100%">STATISTICAL ANALYSIS</style></keyword><keyword><style  face="normal" font="default" size="100%">THERMAL PLASMAS</style></keyword><keyword><style  face="normal" font="default" size="100%">whistlers</style></keyword></keywords><dates><year><style  face="normal" font="default" size="100%">1993</style></year><pub-dates><date><style  face="normal" font="default" size="100%">nov</style></date></pub-dates></dates><volume><style face="normal" font="default" size="100%">98</style></volume><pages><style face="normal" font="default" size="100%">19243</style></pages><language><style face="normal" font="default" size="100%">eng</style></language><reprint-edition><style face="normal" font="default" size="100%">0404</style></reprint-edition></record></records></xml>