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A three‐fluid, 16‐moment gyrotropic bi‐Maxwellian fast solar wind: the effect of He++
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/content/aip/proceeding/aipcp/10.1063/1.1618608
http://aip.metastore.ingenta.com/content/aip/proceeding/aipcp/10.1063/1.1618608
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/content/aip/proceeding/aipcp/10.1063/1.1618608
2003-09-02
2016-05-01

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