On the sources of the night side ionosphere of Venus
Contenido principal del artículo
Resumen
Se presenta una descripción general de las características de la ionósfera nocturna en Venus y del medio magnético y plasmático en su estela. Se sugiere que el carácter variable de la ionósfera nocturna, es debido en parte, a condiciones de asimetría y variaciones temporales de la penetración viscosa del viento solar a la región de la umbra óptica atrás del terminador planetario. Además de Ios efectos de inducción, la presencia de flujos magnéticos asociados con el plasma solar debe contribuir a explicar la dependencia que ejerce el campo magnético interplanetario sobre la geometría magnética dentro de la umbra óptica.
Detalles del artículo
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