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Impactos Cometários na Magnetosfera Joviana

Impactos Cometários na Magnetosfera Joviana

Bipasa Raha / Debojyoti Halder

112,92 €
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Editorial:
KS OmniScriptum Publishing
Año de edición:
2024
Materia
Astronomía, espacio y tiempo
ISBN:
9786208177096
112,92 €
IVA incluido
Disponible

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Sobre IBD

Do ponto de vista dos fenómenos físicos básicos, Júpiter é considerado o mais interessante dos planetas. Com base em provas de rádio, tem uma imensa cintura de radiação de electrões relativistas e um momento magnético mais de 105 vezes superior ao da Terra. A magnetosfera de Júpiter é muito diferente da da Terra no seu funcionamento fundamental. Esta diferença desafia o nosso pensamento e a nossa compreensão da física da magnetosfera e do comportamento da matéria a uma escala cósmica. A magnetosfera da Terra extrai essencialmente toda a sua energia e uma fração significativa do seu plasma do vento solar, enquanto que, por outro lado, a magnetosfera de Júpiter é alimentada pelo abrandamento da rotação de Júpiter e, de facto, aproximadamente todo o seu plasma magnetosférico tem origem em fontes internas, principalmente do satélite-Io e da ionosfera joviana. Além disso, Júpiter exibe um comportamento pulsar fraco mas genuíno. Júpiter funciona de forma diferente de outras magnetosferas e permite alargar as nossas concepções para desenvolver melhores teorias sobre a magnetosfera da Terra. Também se liga a objectos astrofísicos distantes para recolher informações sobre eles em várias formas de deteção remota.

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