Turbulence, Intermittency, and Cross-Scale Energy Transfer in an Interplanetary Coronal Mass Ejection
- Location
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Deutsche Nationalbibliothek Frankfurt am Main
- Extent
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Online-Ressource, 1 online resource.
- Language
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Englisch
- Bibliographic citation
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Turbulence, Intermittency, and Cross-Scale Energy Transfer in an Interplanetary Coronal Mass Ejection ; volume:298 ; number:4 ; day:7 ; month:4 ; year:2023 ; pages:1-16 ; date:4.2023
Solar physics ; 298, Heft 4 (7.4.2023), 1-16, 4.2023
- Creator
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Márquez Rodríguez, Roque
Sorriso-Valvo, Luca
Yordanova, Emiliya
- Contributor
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SpringerLink (Online service)
- DOI
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10.1007/s11207-023-02146-1
- URN
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urn:nbn:de:101:1-2023090516592964957145
- Rights
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Open Access; Der Zugriff auf das Objekt ist unbeschränkt möglich.
- Last update
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14.08.2025, 11:01 AM CEST
Data provider
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Associated
- Márquez Rodríguez, Roque
- Sorriso-Valvo, Luca
- Yordanova, Emiliya
- SpringerLink (Online service)
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Development of a coronal mass ejection arrival time forecasting system using interplanetary scintillation observations
Cosmic noise absorption signature of particle precipitation during interplanetary coronal mass ejection sheaths and ejecta
Statistical analysis of mirror mode waves in sheath regions driven by interplanetary coronal mass ejection
Validation of coronal mass ejection arrival-time forecasts by magnetohydrodynamic simulations based on interplanetary scintillation observations
Three-Dimensional Simulations of Solar Wind Preconditioning and the 23 July 2012 Interplanetary Coronal Mass Ejection
Nanodust dynamics during a coronal mass ejection
Reconnection in a slow Coronal Mass Ejection
Coronal mass ejections and their sheath regions in interplanetary space
Internal characteristics of magnetic clouds and interplanetary coronal mass ejections
Effect of interplanetary shock waves on turbulence parameters
Dynamic coronal mass ejection process and magnetic reconnection
Proton beam velocity distributions in an interplanetary coronal mass ejection
Development of a coronal mass ejection arrival time forecasting system using interplanetary scintillation observations
Cosmic noise absorption signature of particle precipitation during interplanetary coronal mass ejection sheaths and ejecta
Statistical analysis of mirror mode waves in sheath regions driven by interplanetary coronal mass ejection
Validation of coronal mass ejection arrival-time forecasts by magnetohydrodynamic simulations based on interplanetary scintillation observations
Three-Dimensional Simulations of Solar Wind Preconditioning and the 23 July 2012 Interplanetary Coronal Mass Ejection
Nanodust dynamics during a coronal mass ejection
Reconnection in a slow Coronal Mass Ejection
Coronal mass ejections and their sheath regions in interplanetary space
Internal characteristics of magnetic clouds and interplanetary coronal mass ejections
Effect of interplanetary shock waves on turbulence parameters
Dynamic coronal mass ejection process and magnetic reconnection
Proton beam velocity distributions in an interplanetary coronal mass ejection
Development of a coronal mass ejection arrival time forecasting system using interplanetary scintillation observations
Cosmic noise absorption signature of particle precipitation during interplanetary coronal mass ejection sheaths and ejecta
Statistical analysis of mirror mode waves in sheath regions driven by interplanetary coronal mass ejection
Validation of coronal mass ejection arrival-time forecasts by magnetohydrodynamic simulations based on interplanetary scintillation observations
Three-Dimensional Simulations of Solar Wind Preconditioning and the 23 July 2012 Interplanetary Coronal Mass Ejection
Nanodust dynamics during a coronal mass ejection
Reconnection in a slow Coronal Mass Ejection
Coronal mass ejections and their sheath regions in interplanetary space
Internal characteristics of magnetic clouds and interplanetary coronal mass ejections
Effect of interplanetary shock waves on turbulence parameters