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Una barrera impenetrable para los electrones ultrarelativistas en los cinturones de radiación de Van Allen
D N Baker1, A N Jaynes1, V C Hoxie1
1Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Colorado 80303, USA.
Nature
|November 28, 2014
Resumen
Los cinturones de radiación de Van Allen.
Área de la Ciencia:
- Física del espacio Física del espacio.
- La física del plasma es la física del plasma.
- La geofísica es la geofísica.
Sus antecedentes:
- Los cinturones de radiación Van Allen de la Tierra se caracterizan por zonas internas y externas de partículas de alta energía.
- Una región de ranura típicamente separa estas zonas, con electrones de energía moderada poblando ambas.
- La plasmapausa, el límite exterior de la plasmasfera, se ha relacionado con la estructura del cinturón de radiación.
Objetivo del estudio:
- Investigar la morfología inesperada de los cinturones de radiación, particularmente a energías ultrarelativistas.
- Para identificar la causa del agudo límite interno observado para los electrones ultrarelativistas.
- Comprender los mecanismos que limitan el transporte radial hacia adentro de electrones energéticos.
Principales métodos:
- Análisis de un conjunto de datos extendido de observaciones del cinturón de radiación.
- Examen de datos medidos simultáneamente sobre el transporte de partículas y las interacciones de ondas.
- Modelado de los procesos de difusión y dispersión de partículas dentro de la plasmasfera.
Principales resultados:
- Se identificó un límite interno extremadamente agudo para los electrones ultrarelativistas en los cinturones de Van Allen.
- Este límite no es causado por un límite de campo magnético físico o campos de onda del transmisor.
- La difusión radial hacia adentro excepcionalmente lenta y la dispersión persistente de partículas de onda crean una barrera a la migración de electrones energéticos.
Conclusiones:
- El límite agudo interno de la zona de radiación externa es una característica dinámica, no un límite de campo magnético estático.
- Los procesos naturales, específicamente la difusión lenta y la dispersión débil, son responsables de la barrera de electrones observada.
- Comprender estos mecanismos es crucial para predecir el comportamiento de los cinturones de radiación de la Tierra.
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