Walsh, AP; Haaland, S; Forsyth, C; Keesee, AM; Kissinger, J; Li, K; Runov, A; ... Taylor, MGGT; + view all Walsh, AP; Haaland, S; Forsyth, C; Keesee, AM; Kissinger, J; Li, K; Runov, A; Soucek, J; Walsh, BM; Wing, S; Taylor, MGGT; - view fewer (2014) Dawn–dusk asymmetries in the coupled solar wind–magnetosphere–ionosphere system: a review. Annales Geophysicae , 32 (7) pp. 705-737. 10.5194/angeo-32-705-2014.

Preview

Text Forsyth_angeo-32-705-2014.pdf - Published Version Download (5MB) | Preview

Abstract

Dawn–dusk asymmetries are ubiquitous features of the coupled solar-wind–magnetosphere–ionosphere system. During the last decades, increasing availability of satellite and ground-based measurements has made it possible to study these phenomena in more detail. Numerous publications have documented the existence of persistent asymmetries in processes, properties and topology of plasma structures in various regions of geospace. In this paper, we present a review of our present knowledge of some of the most pronounced dawn–dusk asymmetries. We focus on four key aspects: (1) the role of external influences such as the solar wind and its interaction with the Earth's magnetosphere; (2) properties of the magnetosphere itself; (3) the role of the ionosphere and (4) feedback and coupling between regions. We have also identified potential inconsistencies and gaps in our understanding of dawn–dusk asymmetries in the Earth's magnetosphere and ionosphere.

Download activity - last month

Export as CSVXMLJSON

Download activity - last 12 months

Export as CSVJSONXML

Downloads by country - last 12 months

Export as XMLJSONCSV

Archive Staff Only

View Item