E-mail address: b. Use the link below to share a full-text version of this article with your friends and colleagues. Learn. During the first 2.
The unusual Cluster crossing compared to the usual midaltitude cusp crossing at this time of the year occurred owing to a large New Onsala girlfriends of the magnetosphere. Cluster, which was in the southern magnetospheric lobe, suddenly found itself in the magnetosheath at the arrival Kiruna hawkeye online the CME at UT. Cluster then crossed through the compressed magnetosheath highly compressed after the discontinuity in the CME for about 1.
The cusps are also known as favorable regions to observe the signatures of magnetic reconnection [e. Using energetic electrons as field line topology tracers, Zong et al.
The region just equatorward of the cusp opening through which magnetosheath plasma enters the closed field lines through turbulence and diffusion is known as the entry layer EL and the region poleward of the cusp opening through which part of the cusp plasma escapes to the nightside tail lobe hawkeyw known as the plasma mantle PM [ Haerendel et al.
Between the cusp and magnetosheath there is an KKiruna region called exterior cusp. The exterior cusp was predicted by the gas dynamic model of Spreiter and Summers .
Kiruna hawkeye online Lavraud et al. Its external boundary with the magnetosheath has sharp bulk velocity gradient and it appears stagnant under northward IMF conditions while more convective antisunward during southward IMF conditions [ Cargill et al.
The exterior cusp is generally associated with depressed magnetic field and lies predominantly within — MLTs and extends to both hawksye and Disabled dating in Stockholm MLTs [e.
Since the exterior cusps are regions where plasma pressure and magnetic field pressure balance [ Cargill et al. Gopalswamy et al. The papers describe the solar sources, propagation and energetic particle distribution of the CMEs. The geoeffectiveness of the CMEs including their impacts on the magnetosphere, and effects on the ionosphere, thermosphere and atmosphere are also described in hawkey number of papers [e.
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An extremely large solar eruption on 28 October caused an intense geomagnetic storm, and a second solar eruption on 29 October resulted in a reintensification of the geomagnetic storm about a day later. Within the second storm, some of the strongest substorms in the history of magnetic recordings occurred in northern Scandinavia, and geomagnetically induced currents in ground conductors caused power failures for 20 to 50 min in southern Sweden [ Rosenqvist et al.
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Observations and Discussion 4.
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However, it is noted that, while this behavior is well pronounced in the case of duskward IMF, the dawnward IMF case shows a more complex structure, in particular near the equatorward boundary. Reply send.
By use of the Shue et al. Ness and P.
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Response of the magnetosheath‐cusp region to a coronal mass ejection
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