Momentum flux of the solar wind near planetary magnetospheres: a comparative study
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Se presenta un estudio del perfil Je velocidad del viento solar exterior a las magnetosferas de laTierra, Marte y Venus. Existe una diferencia característica en las condiciones presentes en planetas con magnetización interna alta y débil. En el caso de un planeta fuertemente magnetizado, como lo es la Tierra, la velocidad del viento solar cerca de la magnetopausa se mantiene aproximadamente constante en la dirección normal a esa frontera. En planetas de baja magnetización (Venus, Marte) el perfil de velocidad muestra, cerca de la magnetoionopausa, un gradiente transversal el cual implica una reducción efectiva del flujo de momento del viento solar en esa región. El diferente comportamiento del viento solar en la vecindad de cada planeta es examinado en conexión con el proceso de interacción que opera en su frontera magnetosférica.
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