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Cómo Explorar el Explorador 3D de Heliosismología y Oscilación Solar

Abre el Explorador 3D de Heliosismología y Oscilación Solar, observa la superficie ondulante y luego activa el corte interior para ver el límite real medido que este patrón de ondulación ayuda a encontrar a los astrónomos.

  1. Abre https://freetoolonline.com/space-3d/helioseismology-sun-oscillation.html y espera a que aparezcan la esfera ondulante y el panel de datos.
  2. Arrastra el control de amplitud de onda para hacer el patrón más fácil o más difícil de ver.
  3. Haz clic en "Next wave pattern" para alternar entre tres patrones de oscilación simplificados.
  4. Haz clic en "Show interior cutaway" para ver un corte transversal con el límite medido de 0,713 radios solares y la tachocline.
  5. Arrastra para orbitar y desliza o pinza para acercar y ver más de cerca.
  6. Lee el panel de datos para conocer el período de oscilación, el número de modos y los límites medidos.

Cifras publicadas clave

CifraValor
Período de oscilaciónunos 5 minutos (unos 3 mHz)
Modos resonantes rastreadosmillones, mediante SOHO / GONG / SDO-HMI
Base medida de la zona de convección0,713 +/- 0,001 radios solares
Ubicación de la tachoclineentre 0,69 y 0,72 radios solares; espesor de unos 0,006-0,05 radios solares

Siguiente: la guía de cuándo usarlo o comparación con alternativas. Abre el Explorador 3D de Heliosismología y Oscilación Solar.

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