Coronal Holes, Footpoint Reconnection, and the Origin of the Slow (and Fast) Solar Wind
- Location
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Deutsche Nationalbibliothek Frankfurt am Main
- Extent
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1 Online-Ressource.
- Language
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Englisch
- Bibliographic citation
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Coronal Holes, Footpoint Reconnection, and the Origin of the Slow (and Fast) Solar Wind ; volume:299 ; number:4 ; day:23 ; month:4 ; year:2024 ; pages:1-19 ; date:4.2024
Solar physics ; 299, Heft 4 (23.4.2024), 1-19, 4.2024
- Creator
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Wang, Y.-M
- Contributor
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SpringerLink (Online service)
- DOI
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10.1007/s11207-024-02300-3
- URN
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urn:nbn:de:101:1-2407152103463.263922016999
- Rights
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Open Access; Der Zugriff auf das Objekt ist unbeschränkt möglich.
- Last update
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14.08.2025, 11:04 AM CEST
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Associated
- Wang, Y.-M
- SpringerLink (Online service)
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Physical mechanism of spontaneous fast reconnection evolution
Particle Acceleration Due to Coronal Non-null Magnetic Reconnection
Origin of resistivity in reconnection
Solar coronal holes observed with SOHO
Conditions for substorm onset by the fast reconnection mechanism
Topologically driven coronal dynamics – a mechanism for coronal hole jets
Observationally quantified reconnection providing a viable mechanism for active region coronal heating
Global destabilization due to localized reconnection: A mechanism for coronal mass ejections
Reconnection in a slow Coronal Mass Ejection
Coronal Holes
Signatures of Coronal Loop Opening via Interchange Reconnection in the Slow Solar Wind at 1 AU
Dynamic coronal mass ejection process and magnetic reconnection
Physical mechanism of spontaneous fast reconnection evolution
Particle Acceleration Due to Coronal Non-null Magnetic Reconnection
Origin of resistivity in reconnection
Solar coronal holes observed with SOHO
Conditions for substorm onset by the fast reconnection mechanism
Topologically driven coronal dynamics – a mechanism for coronal hole jets
Observationally quantified reconnection providing a viable mechanism for active region coronal heating
Global destabilization due to localized reconnection: A mechanism for coronal mass ejections
Reconnection in a slow Coronal Mass Ejection
Coronal Holes
Signatures of Coronal Loop Opening via Interchange Reconnection in the Slow Solar Wind at 1 AU
Dynamic coronal mass ejection process and magnetic reconnection
Physical mechanism of spontaneous fast reconnection evolution
Particle Acceleration Due to Coronal Non-null Magnetic Reconnection
Origin of resistivity in reconnection
Solar coronal holes observed with SOHO
Conditions for substorm onset by the fast reconnection mechanism
Topologically driven coronal dynamics – a mechanism for coronal hole jets
Observationally quantified reconnection providing a viable mechanism for active region coronal heating