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10.1038/nphys3879 http://scihub22266oqcxt.onion/10.1038/nphys3879 C5131847!5131847 !27917231     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 Warning: imagejpeg(C:\Inetpub\vhosts\kidney.de\httpdocs\phplern\27917231 .jpg): Failed to open stream: No such file or directory in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 117       Nat+Phys 2016 ; 12 (12 ): 1158-1163 Nephropedia Template TP {{tp|p=27917231 |t=2016. Magnetotail energy dissipation during an auroral substorm |pdf=|usr=}}{{27917231 }} gab.com Text Magnetotail energy dissipation during an auroral substorm JO: Nat Phys http://www.kidney.de/pget.php?&tw=1&pmid=27917231 #FOAvip Violent releases of space plasma energy from the Earth's magnetotail during substorms produce strong electric currents and bright aurora. But what modulates these currents and aurora and controls dissipation of the energy released in the ionosphere? Using data from the THEMIS fleet of satellites and ground-based imagers and magnetometers, we show that plasma energy dissipation is controlled by field-aligned currents (FACs) produced and modulated during magnetotail topology change and oscillatory braking of fast plasma jets at 10-14 Earth radii in the nightside magnetosphere. FACs appear in regions where plasma sheet pressure and flux tube volume gradients are non-collinear. Faster tailward expansion of magnetotail dipolarization and subsequent slower inner plasma sheet restretching during substorm expansion and recovery phases cause faster poleward then slower equatorward movement of the substorm aurora. Anharmonic radial plasma oscillations build up displaced current filaments and are responsible for discrete longitudinal auroral arcs that move equatorward at a velocity of about 1km/s. This observed auroral activity appears sufficient to dissipate the released energy. Twit Text FOAVip Magnetotail energy dissipation during an auroral substorm ????Nat Phys http://www.kidney.de/pget.php?&tw=1&pmid=27917231 #FOAvip Twit Text # Free Paper on # # # # # LINK http://www.kidney.de/pget.php?&tw=1&pmid=27917231 #FOAvip English Wikipedia <ref>{{Cite pmid|27917231 }}</ref> Magnetotail energy dissipation during an auroral substorm #MMPMID27917231 Panov EV ; Baumjohann W ; Wolf RA ; Nakamura R ; Angelopoulos V ; Weygand JM ; Kubyshkina MV Nat Phys 2016[Dec]; 12 (12 ): 1158-1163 PMID27917231 show ga Violent releases of space plasma energy from the Earth's magnetotail during substorms produce strong electric currents and bright aurora. But what modulates these currents and aurora and controls dissipation of the energy released in the ionosphere? Using data from the THEMIS fleet of satellites and ground-based imagers and magnetometers, we show that plasma energy dissipation is controlled by field-aligned currents (FACs) produced and modulated during magnetotail topology change and oscillatory braking of fast plasma jets at 10-14 Earth radii in the nightside magnetosphere. FACs appear in regions where plasma sheet pressure and flux tube volume gradients are non-collinear. Faster tailward expansion of magnetotail dipolarization and subsequent slower inner plasma sheet restretching during substorm expansion and recovery phases cause faster poleward then slower equatorward movement of the substorm aurora. Anharmonic radial plasma oscillations build up displaced current filaments and are responsible for discrete longitudinal auroral arcs that move equatorward at a velocity of about 1km/s. This observed auroral activity appears sufficient to dissipate the released energy. äMagnetotail energy dissipation during an auroral substorm (epmc).pdf DeepDyve Pubget Overpricing