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| Titel |
Are there current-sheet-like structures in the Earth's magnetotail as in the solar wind – results and implications from high time resolution magnetic field measurements by Cluster |
| VerfasserIn |
G. Li, E. Lee, G. Parks |
| Medientyp |
Artikel
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| Sprache |
Englisch
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| ISSN |
0992-7689
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| Digitales Dokument |
URL |
| Erschienen |
In: Annales Geophysicae ; 26, no. 7 ; Nr. 26, no. 7 (2008-07-14), S.1889-1895 |
| Datensatznummer |
250016154
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| Publikation (Nr.) |
 copernicus.org/angeo-26-1889-2008.pdf |
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| Zusammenfassung |
| Recent studies of solar wind MHD turbulence show that current-sheet-like structures
are common in the solar wind and they are a significant source of solar wind MHD turbulence
intermittency.
While numerical simulations have suggested that such structures can arise
from non-linear interactions of MHD turbulence, a recent study by Borovsky
(2006), upon
analyzing one year worth of ACE data, suggests that these structures may represent
the magnetic walls of flux tubes that separate solar wind plasma into distinct bundles
and these flux tubes are relic structures originating from boundaries of supergranules
on the surface of the Sun. In this work,
we examine whether there are such structures in the Earth's magnetotail,
an environment vastly different from the solar wind.
We use high time resolution magnetic field data of the FGM instrument onboard Cluster C1 spacecraft.
The orbits of Cluster traverse through both the solar wind and the Earth's
magnetosheath and magnetotail. This makes its dataset ideal for studying differences between
solar wind MHD turbulence and that inside the Earth's magnetosphere.
For comparison, we also perform the same analysis when Cluster C1 is in the solar wind.
Using a data analysis procedure first introduced in Li (2007, 2008), we
find that current-sheet-like structures can be clearly identified
in the solar wind. However, similar structures do not exist inside the Earth's
magnetotail.
This result can be naturally explained if these structures have a solar origin as
proposed by Borovsky (2006).
With such a scenario, current analysis of solar wind MHD turbulence needs to be improved to
include the effects due to these curent-sheet-like structures. |
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