Dusty plasma in space

Contenido principal del artículo

N. Ya. Kotsarenko
S. V. Koshevaya
A. N. Kotsarenko

Resumen

Intensos estudios de la física de plasmas realizados desde hace alrededor de 10 años han visto el surgimiento de una nueva línea de investigación: la física de plasmas polvosos, que consisten de electrones, iones y partículas de polvo cargadas. Se observan en varios medios astrofísicos como nebulosas, colas cometarias, anillos planetarios, ionosferas planetarias, etc. La presencia de partículas de polvo pesadas y cargadas puede influenciar significativamente varios parámetros del plasma al crear, por ejemplo, estructuras en su interior en un rango muy amplio de cientos a decenas de millones de kilómetros. En este trabajo presentamos una revisión y un análisis del espectro del volumen y ondas superficiales, estabilidades y solitones en un plasma polvoso.

Detalles del artículo

Cómo citar
Kotsarenko, N. Y., Koshevaya, S. V., & Kotsarenko, A. N. (1998). Dusty plasma in space. Geofísica Internacional, 37(2), 71–86. https://doi.org/10.22201/igeof.00167169p.1998.37.2.396
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