Röken, Christian ; Kleimann, Jens 
; Fichtner, Horst
Alternative Links zum Volltext:DOIVerlag
| Dokumentenart: | Artikel |
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| Titel eines Journals oder einer Zeitschrift: | The Astrophysical Journal |
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| Verlag: | IOP PUBLISHING LTD |
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| Ort der Veröffentlichung: | BRISTOL |
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| Band: | 805 |
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| Nummer des Zeitschriftenheftes oder des Kapitels: | 2 |
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| Seitenbereich: | S. 173 |
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| Datum: | 2015 |
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| Institutionen: | Mathematik |
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| Identifikationsnummer: | | Wert | Typ |
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| 10.1088/0004-637X/805/2/173 | DOI |
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| Stichwörter / Keywords: | TEV COSMIC-RAYS; SOLAR-WIND; BOW SHOCK; GLOBAL HELIOSPHERE; OUTER HELIOSPHERE; VOYAGER 1; HELIOPAUSE; HELIOSHEATH; ANISOTROPY; MODULATION; ISM: magnetic fields; magnetohydrodynamics (MHD); methods: analytical; Sun: heliosphere |
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| Dewey-Dezimal-Klassifikation: | 500 Naturwissenschaften und Mathematik > 510 Mathematik |
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| Status: | Veröffentlicht |
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| Begutachtet: | Ja, diese Version wurde begutachtet |
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| An der Universität Regensburg entstanden: | Ja |
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| Dokumenten-ID: | 60358 |
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Zusammenfassung
An analytical representation of the interstellar magnetic field in the vicinity of the heliosphere is derived. The three-dimensional field structure close to the heliopause is calculated as a solution of the induction equation under the assumption that it is frozen into a prescribed plasma flow resembling the characteristic interaction of the solar wind with the local interstellar medium. The ...
Zusammenfassung
An analytical representation of the interstellar magnetic field in the vicinity of the heliosphere is derived. The three-dimensional field structure close to the heliopause is calculated as a solution of the induction equation under the assumption that it is frozen into a prescribed plasma flow resembling the characteristic interaction of the solar wind with the local interstellar medium. The usefulness of this analytical solution as an approximation to self-consistent magnetic field configurations obtained numerically from the full MHD equations is illustrated by quantitative comparisons.
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