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Las emisiones de gases y las erupciones del Monte St. Helens hasta 1982
Resumen
El monitoreo del Monte St. Helens.
Área de la Ciencia:
- Vulcanología y geoquímica.
Sus antecedentes:
- El Monte St. Helens tiene emisiones continuas de gases.
- La composición de los gases volcánicos y las tasas de emisión proporcionan información sobre los procesos magmáticos.
Objetivo del estudio:
- Para analizar las emisiones de gases del Monte St. Helens.
- Para comprender los procesos magmáticos y predecir la actividad volcánica.
Principales métodos:
- Medidas diarias en el aire del dióxido de azufre en el penacho volcánico.
- Muestreo mensual de gases de las fumarolas del cráter.
Principales resultados:
- La composición del gas fumarolico cambió: el agua aumentó (90-98%), el dióxido de carbono disminuyó (10-1%).
- Las tasas de emisión de dióxido de azufre y dióxido de carbono alcanzaron su punto máximo a mediados de 1980, luego disminuyeron y se estabilizaron.
- Los datos de gas predijeron con éxito erupciones en agosto de 1980 y junio de 1981.
Conclusiones:
- Los patrones de gas observados sugieren una desgasificación constante de un solo lote de magma desde mediados de 1980.
- No se ha producido ningún nuevo flujo de magma significativo desde mediados de 1980.
- El monitoreo de gases es una herramienta valiosa para la predicción de erupciones en el Monte St. Helens.
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