Heliosfera

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L'Heliosfera.

L'Heliosfera (d'o griego ἥλιος sol y σφαῖρα esfera) ye a vasta rechión de l'espacio en forma de bambolla que rodeya y ye creyada por o Sol.[1] En termins d'a fisica d'o plasma, ye a cavidat formada por o Sol en o medio interestelar circumdant. A "bambolla" de l'heliosfera se "rinfla" de contino por o plasma que s'orichina en o Sol, conoixiu como aire solar. Difuera de l'heliosfera, iste plasma solar da paso a lo plasma interestelar que permia a Carrera de sant Chaime. Os livels de radiación adintro y difuera de l'heliosfera difieren; en particular, os rayos cosmicos galacticos son menos abundants dentro de l'heliosfera, por o que as planetas de l'interior (incluida a Tierra) son parcialment protechius d'o suyo impauto.

Se diz que a parola "heliosfera" estió cudida por Alexander J. Dessler, a qui se le atribuye o primer uso d'a parola en a literatura cientifica en 1967. L'estudio cientifico de l'heliosfera ye a heliofisica, que incluye l'orache espacial y o clima espacial.

Referencias

  1. ↑ (en) Joseph A. Angelo Jr. Encyclopedia of Space and Astronomy, Facts on File, 2006, ISBN 978-0-8160-5330-8, p.291

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