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10.1038/srep23497 http://scihub22266oqcxt.onion/10.1038/srep23497 C4804308!4804308!27005472     free     free     free Deprecated: Implicit conversion from float 211.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 211.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534       Sci+Rep 2016 ; 6 (ä): ä Nephropedia Template TP {{tp|p=27005472|t=2016. Using Jupiter?s gravitational field to probe the Jovian convective dynamo |pdf=|usr=}}{{27005472}} gab.com Text Using Jupiter s gravitational field to probe the Jovian convective dynamo JO: Sci Rep http://www.kidney.de/pget.php?&tw=1&pmid=27005472 #FOAvip Convective motion in the deep metallic hydrogen region of Jupiter is believed to generate its magnetic field, the strongest in the solar system. The amplitude, structure and depth of the convective motion are unknown. A promising way of probing the Jovian convective dynamo is to measure its effect on the external gravitational field, a task to be soon undertaken by the Juno spacecraft. We calculate the gravitational signature of non-axisymmetric convective motion in the Jovian metallic hydrogen region and show that with sufficiently accurate measurements it can reveal the nature of the deep convection. Twit Text FOAVip Using Jupiter s gravitational field to probe the Jovian convective dynamo ????Sci Rep http://www.kidney.de/pget.php?&tw=1&pmid=27005472 #FOAvip Twit Text # Free Paper on # # # # # LINK http://www.kidney.de/pget.php?&tw=1&pmid=27005472 #FOAvip English Wikipedia <ref>{{Cite pmid|27005472}}</ref> Using Jupiter?s gravitational field to probe the Jovian convective dynamo #MMPMID27005472 Kong D; Zhang K; Schubert G Sci Rep 2016[]; 6 (ä): ä PMID27005472show ga Convective motion in the deep metallic hydrogen region of Jupiter is believed to generate its magnetic field, the strongest in the solar system. The amplitude, structure and depth of the convective motion are unknown. A promising way of probing the Jovian convective dynamo is to measure its effect on the external gravitational field, a task to be soon undertaken by the Juno spacecraft. We calculate the gravitational signature of non-axisymmetric convective motion in the Jovian metallic hydrogen region and show that with sufficiently accurate measurements it can reveal the nature of the deep convection. äUsing Jupiter?s gravitational field to probe the Jovian convective dyn(epmc).pdf DeepDyve Pubget Overpricing