Evidence for impulsive solar wind plasma penetration through the dayside magnetopause

R. Lundin (1, 2) , J.-A. Sauvaud (1) , H. Rème (1) , A. Balogh (3) , I. Dandouras (1) , J. M. Bosqued (1) , C. Carlson (4) , G. K. Parks (4) , E. Möbius (5) , L. M. Kistler (5) , B. Klecker (6) , E. Amata (7) , V. Formisano (7) , M. Dunlop (3) , L. Eliasson (2) , A. Korth (8) , B. Lavraud (1) , M. Mccarthy (9)

1 CESR - Centre d'étude spatiale des rayonnements
2 IRF - Swedish Institute of Space Physics [Kiruna]
3 Imperial College London
4 SSL - Space Sciences Laboratory [Berkeley]
5 EOS - Institute for the Study of Earth, Oceans, and Space [Durham]
6 MPE - Max-Planck-Institut für Extraterrestrische Physik
7 IFSI - Istituto di Fisica dello Spazio Interplanetario
8 MPI Aeronomie - Max-Planck-Institut für Aeronomie
9 Space Program

This paper presents in situ observational evidence from the Cluster Ion Spectrometer (CIS) on Cluster of injected solar wind "plasma clouds" protruding into the day-side high-latitude magnetopause. The plasma clouds, presumably injected by a transient process through the day-side magnetopause, show characteristics implying a generation mechanism denoted impulsive penetration (Lemaire and Roth, 1978).

The injected plasma clouds, hereafter termed "plasma transfer events", (PTEs), (Woch and Lundin, 1991), are temporal in nature and relatively limited in size. They are initially moving inward with a high velocity and a magnetic signature that makes them essentially indistinguishable from regular magnetosheath encounters. Once inside the magnetosphere, however, PTEs are more easily distinguished from magnetopause encounters. The PTEs may still be moving while embedded in an isotropic background of energetic trapped particles but, once inside the magnetosphere, they expand along magnetic field lines. However, they frequently have a significant transverse drift component as well. The drift is localised, thus constituting an excess momentum/motional emf generating electric fields and currents. The induced emf also acts locally, accelerating a pre-existing cold plasma (e.g. Sauvaud et al., 2001). Observations of PTE-signatures range from "active" (strong transverse flow, magnetic turbulence, electric current, local plasma acceleration) to "evanescent" (weak flow, weak current signature).

PTEs appear to occur independently of Interplanetary Magnetic Field (IMF) Bz in the vicinity of the polar cusp region, which is consistent with observations of transient plasma injections observed with mid- and high-altitude satellites (e.g. Woch and Lundin, 1992; Stenuit et al., 2001). However the characteristics of PTEs in the magnetosphere boundary layer differ for southward and northward IMF. The Cluster data available up to now indicate that PTEs penetrate deeper into the magnetosphere for northward IMF than for southward IMF. This may or may not mark a difference in nature between PTEs observed for southward and northward IMF. Considering that flux transfer events (FTEs), (Russell and Elphic, 1979), are observed for southward IMF or when the IMF is oriented such that antiparallel merging may occur, it seems likely that PTEs observed for southward IMF are related to FTEs.

Domaines: Océan, Atmosphère; Sciences de la Terre

R. Lundin, J.-A. Sauvaud, H. Rème, A. Balogh, I. Dandouras, et al.. Evidence for impulsive solar wind plasma penetration through the dayside magnetopause. Annales Geophysicae, 2003, 21 (2), pp.457-472. ⟨hal-00329232⟩