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10.1038/ncomms7491 http://scihub22266oqcxt.onion/10.1038/ncomms7491 C4396379!4396379!25849045     free     free     free Deprecated: Implicit conversion from float 231.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 231.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 231.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 231.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 231.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534       Nat+Commun ä ; 6 (ä): ä Nephropedia Template TP {{tp|p=25849045|t=ä. The solar magnetic activity band interaction and instabilities that shape quasi-periodic variability |pdf=|usr=}}{{25849045}} gab.com Text The solar magnetic activity band interaction and instabilities that shape quasi-periodic variability JO: Nat Commun http://www.kidney.de/pget.php?&tw=1&pmid=25849045 #FOAvip Solar magnetism displays a host of variational timescales of which the enigmatic 11-year sunspot cycle is most prominent. Recent work has demonstrated that the sunspot cycle can be explained in terms of the intra- and extra-hemispheric interaction between the overlapping activity bands of the 22-year magnetic polarity cycle. Those activity bands appear to be driven by the rotation of the Sun's deep interior. Here we deduce that activity band interaction can qualitatively explain the ?Gnevyshev Gap'?a well-established feature of flare and sunspot occurrence. Strong quasi-annual variability in the number of flares, coronal mass ejections, the radiative and particulate environment of the heliosphere is also observed. We infer that this secondary variability is driven by surges of magnetism from the activity bands. Understanding the formation, interaction and instability of these activity bands will considerably improve forecast capability in space weather and solar activity over a range of timescales. Twit Text FOAVip The solar magnetic activity band interaction and instabilities that shape quasi-periodic variability ????Nat Commun http://www.kidney.de/pget.php?&tw=1&pmid=25849045 #FOAvip Twit Text # Free Paper on # # # # # LINK http://www.kidney.de/pget.php?&tw=1&pmid=25849045 #FOAvip English Wikipedia <ref>{{Cite pmid|25849045}}</ref> The solar magnetic activity band interaction and instabilities that shape quasi-periodic variability #MMPMID25849045 McIntosh SW; Leamon RJ; Krista LD; Title AM; Hudson HS; Riley P; Harder JW; Kopp G; Snow M; Woods TN; Kasper JC; Stevens ML; Ulrich RK Nat Commun ä[]; 6 (ä): ä PMID25849045show ga Solar magnetism displays a host of variational timescales of which the enigmatic 11-year sunspot cycle is most prominent. Recent work has demonstrated that the sunspot cycle can be explained in terms of the intra- and extra-hemispheric interaction between the overlapping activity bands of the 22-year magnetic polarity cycle. Those activity bands appear to be driven by the rotation of the Sun's deep interior. Here we deduce that activity band interaction can qualitatively explain the ?Gnevyshev Gap'?a well-established feature of flare and sunspot occurrence. Strong quasi-annual variability in the number of flares, coronal mass ejections, the radiative and particulate environment of the heliosphere is also observed. We infer that this secondary variability is driven by surges of magnetism from the activity bands. Understanding the formation, interaction and instability of these activity bands will considerably improve forecast capability in space weather and solar activity over a range of timescales. äThe solar magnetic activity band interaction and instabilities that sh(epmc).pdf DeepDyve Pubget Overpricing