Planetary andSdgR SdgRR 50 (2002) 601 -- 612

Abstract

Large (from tens of percent up to several times) ion #ux (or density) and magnetic #eld magnitude variations are typical magnetosheath features. Case and statistical comparisons of simultaneous solar wind observations, magnetosheath observations, and the gasdynamic model for the magnetosheath #ow ofSgD9L9R et al