Plasma channels in the Venus upper ionosphere

Plasma channels in the Venus upper ionosphere

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Se modela la estructura de la ionosfera nocturna del planeta Venus con base en una configuración de flujo derivada de la posición de la transición intermedia en la región de transición con el viento solar. Se infiere que el viento solar erosiona la ionosfera del planeta alrededor de las regiones mag...

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Bibliographic Details
Main Author:	H. Pérez de Tejada
Format:	Article
Language:	English
Published:	Universidad Nacional Autónoma de México, Instituto de Geofísica 2001-01-01
Series:	Geofísica Internacional
Subjects:	ionosfera de venus canales de plasma agujeros ionosféricos
Online Access:	http://revistagi.geofisica.unam.mx/index.php/RGI/article/view/715

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