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Anomalías magnéticas lunares y propiedades ópticas de la superficie lunar
Science (New York, N.Y.)
|April 4, 1980
Resumen
Las fuertes anomalías magnéticas lunares crean vacíos de plasma, lo que sugiere que el bombardeo de iones del viento solar influye en la Luna.
Área de la Ciencia:
- La ciencia lunar es la ciencia lunar.
- Física del espacio Física del espacio
- Geología planetaria Geología planetaria.
Sus antecedentes:
- La Luna posee anomalías magnéticas localizadas.
- El viento solar es una corriente de partículas cargadas procedentes del Sol.
- Las características de la superficie de la Luna exhiben albedo (reflectividad) variable.
Objetivo del estudio:
- Para investigar la interacción entre las anomalías magnéticas lunares y el viento solar.
- Explorar el vínculo potencial entre las anomalías magnéticas, los vacíos de plasma y las propiedades ópticas de la superficie.
Principales métodos:
- Análisis de la desviación del viento solar por los campos magnéticos.
- Correlación de la fuerza de la anomalía magnética con las características de las características de la superficie.
Principales resultados:
- Las anomalías magnéticas lunares con momentos dipolares mayores a 5 x 1013 G cm3 desvían significativamente el viento solar.
- Esta deflexión crea vacíos de plasma localizados en la superficie lunar.
- Las anomalías más fuertes (aprox. 10^16 G cm3) se correlacionan con las características de la superficie de alto albedo.
Conclusiones:
- El bombardeo de iones del viento solar es un factor significativo que da forma a las propiedades ópticas de la superficie de la Luna.
- Las anomalías magnéticas juegan un papel crucial en la modulación de las interacciones entre el viento solar y la superficie.
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