American English Male Voice
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Middle Aged (35-54)Accents
North American (General)Transcript
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their results currently available in a pre print, that has been accepted to nature, harmonized with what cassini saw at Saturn Editor's note that paper has now been published. The results have been taken as hard proof that the auroras can solve the energy crisis. It's a big step forward seeing that it's auroral heating, said Rosie johnson, a space physics researcher at Aberystwyth University in Wales, who wasn't involved with either paper, lisa Ray, a space and planetary physics researcher at Lancaster University in England, who is also not involved with either paper praises the Saturn studies, rigorous data set, but she is less convinced by the jupiter paper. They're only using two nights of data and I find that to be an issue, she said. But despite her misgivings, I think the temperature gradient result at jupiter probably will hold because they've seen it at Saturn, she said, having comparatively few observations is a fair concern because these are very dynamic places, these giant planets said more additional nights of jupiter observations have been collected and are currently being processed in any event. Most independent researchers seem convinced that the planet wide fevers are down to the auroras. These papers provide a really nice confirmation that what we suspected was happening is actually happening, said Lee FLetcher, a planetary scientist at the University of Leicester in England, who was not involved with the work. Energy is leaking from the auroral domain down into the lower latitudes. The question is how the wicked western winds, the majority of atmospheric circulation models struggle to move heat from the aurora through jupiter and Saturn screeching westward winds to the equator at yet their heat maps show that these tempestuous hurdles are somehow being overcome. One potential solution was inspired by CAssini's observations, CAssini discovered that on occasion a disturbance to a lower layer of Saturn's atmosphere can cause that layer to migrate to the upper atmosphere. Such an inversion may disrupt and slow down the upper atmospheres powerful westward winds, perhaps enough to allow the auroral heat to leak through