Duba wurin da ke ƙasa sannan ka amsa tambayar daga baya a cikin harshe ɗaya kamar yadda wurin yake:  Hanyar wucewa: Babbar matsalar da aka fuskanta wajen fassara yanayin yanayin magnetosphere na Jovian shine jigilar plasma mai sanyi mai nauyi daga Io torus a 6 RJ zuwa magnetosphere na waje a nesa fiye da 50 RJ. Ba a san ainihin tsarin wannan tsari ba, amma ana zaton ya faru ne sakamakon yaduwar plasma saboda rashin daidaito na musayar. Tsarin yana kama da rashin kwanciyar hankali na Rayleigh-Taylor a cikin hydrodynamics. A cikin yanayin magnetosphere na Jovian, ƙarfin centrifugal yana taka rawar nauyi; ruwa mai nauyi shine sanyi da Ionian (watau na Io) plasma, kuma ruwa mai haske shine zafi, plasma mai ƙarancin ƙarfi daga magnetosphere na waje. Rashin kwanciyar hankali yana haifar da musayar tsakanin sassan waje da na ciki na magnetosphere na bututun mai cike da plasma. Bututun bututun da ba shi da komai yana motsawa zuwa duniyar, yayin tura bututun mai nauyi, cike da plasma na Ionian, daga Jupiter. Wannan musayar tubes na flux wani nau'i ne na turbulence na magnetospheric.  Tambaya: Wace duniya ce ta biyar?
Jupiter