SM13A-2467
Magnetopause-Foreshock Interactions Induced by Dayside Reconnection

Monday, 14 December 2015
Poster Hall (Moscone South)
Yann Pfau-Kempf1,2, Heli Hietala3, Sanni Hoilijoki1,2, Minna Palmroth1, Urs Ganse2, Arto Sandroos1, Otto Hannuksela1,2, Sebastian von Alfthan1,4 and Rami O Vainio5, (1)Finnish Meteorological Institute, Helsinki, Finland, (2)University of Helsinki, Department of Physics, Helsinki, Finland, (3)Imperial College London, London, United Kingdom, (4)CSC Centre for Scientific Computing, Espoo, Finland, (5)University of Turku, Department of Physics and Astronomy, Turku, Finland
Abstract:
We investigate the effects of dayside reconnection events on the bow shock in global hybrid-Vlasov simulations of the terrestrial magnetosphere. Using the Finnish Meteorological Institute's hybrid-Vlasov model Vlasiator (http://vlasiator.fmi.fi), which couples kinetic ions through Vlasov's equation with charge-neutralizing fluid electrons, the solar wind-magnetosphere interaction is modeled self-consistently in two spatial and three velocity dimensions. Recent polar plane simulations with southward IMF cover both the dayside and nightside reconnection sites, in a volume ranging from about 40 Earth radii (RE) upstream in the solar wind to about one hundred RE tailward.

Dayside reconnection at the magnetopause results in the formation of the two-dimensional equivalents of flux transfer events. These magnetic islands are accelerated and move from the subsolar region towards the cusps and beyond. In doing so, they generate fast-mode waves which propagate throughout the magnetosheath and can lead to significant perturbations in the bow shock shape and position. We investigate such simulated events and their signatures in the magnetosheath, at the bow shock and in the foreshock. We also analyze observational data to find similar signatures in spacecraft measurements.