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| Titel |
Two-spacecraft reconstruction of a magnetic cloud and comparison to its solar source |
| VerfasserIn |
C. Möstl, C. Miklenic, C. J. Farrugia, M. Temmer, A. Veronig, A. B. Galvin, B. Vršnak, H. K. Biernat |
| 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. 10 ; Nr. 26, no. 10 (2008-10-15), S.3139-3152 |
| Datensatznummer |
250016260
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| Publikation (Nr.) |
 copernicus.org/angeo-26-3139-2008.pdf |
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| Zusammenfassung |
| This paper compares properties of the source region with those inferred from
satellite observations near Earth of the magnetic cloud which reached 1 AU on 20 November 2003.
We use observations from space missions SOHO and TRACE together with ground-based data to study the magnetic
structure of the active region NOAA 10501 containing a highly curved filament,
and determine the reconnection rates and fluxes in an M4 flare on 18 November 2003
which is associated with a fast halo CME. This event has been linked before to the
magnetic cloud on 20 November 2003. We model the near-Earth observations with the
Grad-Shafranov reconstruction technique using a novel approach in which we optimize
the results with two-spacecraft measurements of the solar wind plasma and magnetic field made by ACE and WIND.
The two probes were separated by hundreds of Earth radii. They pass through the axis
of the cloud which is inclined −50 degree to the ecliptic.
The magnetic cloud orientation at 1 AU is consistent with an
encounter with the heliospheric current sheet. We estimate that
50% of its poloidal flux has been lost through reconnection in
interplanetary space. By comparing the flare ribbon flux with the
original cloud fluxes we infer a flux rope formation during the
eruption, though uncertainties are still significant. The
multi-spacecraft Grad-Shafranov method opens new vistas in probing
of the spatial structure of magnetic clouds in STEREO-WIND/ACE
coordinated studies. |
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