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10.1002/2017GL073048 http://scihub22266oqcxt.onion/10.1002/2017GL073048 C5488625!5488625!28713180     free     free     free Deprecated: Implicit conversion from float 233.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 233.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 233.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 233.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 233.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 233.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 233.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 233.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 267.2 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534       Geophys+Res+Lett 2017 ; 44 (8): 3456-64 Nephropedia Template TP {{tp|p=28713180|t=2017. Global observations of magnetospheric high?m poloidal waves during the 22 June 2015 magnetic storm |pdf=|usr=}}{{28713180}} gab.com Text Global observations of magnetospheric high m poloidal waves during the 22 June 2015 magnetic storm JO: Geophys Res Lett http://www.kidney.de/pget.php?&tw=1&pmid=28713180 #FOAvip We report global observations of high?m poloidal waves during the recovery phase of the 22 June 2015 magnetic storm from a constellation of widely spaced satellites of five missions including Magnetospheric Multiscale (MMS), Van Allen Probes, Time History of Events and Macroscale Interactions during Substorm (THEMIS), Cluster, and Geostationary Operational Environmental Satellites (GOES). The combined observations demonstrate the global spatial extent of storm time poloidal waves. MMS observations confirm high azimuthal wave numbers (m ~ 100). Mode identification indicates the waves are associated with the second harmonic of field line resonances. The wave frequencies exhibit a decreasing trend as L increases, distinguishing them from the single?frequency global poloidal modes normally observed during quiet times. Detailed examination of the instantaneous frequency reveals discrete spatial structures with step?like frequency changes along L. Each discrete L shell has a steady wave frequency and spans about 1 RE, suggesting that there exist a discrete number of drift?bounce resonance regions across L shells during storm times. Twit Text FOAVip Global observations of magnetospheric high m poloidal waves during the 22 June 2015 magnetic storm ????Geophys Res Lett http://www.kidney.de/pget.php?&tw=1&pmid=28713180 #FOAvip Twit Text # Free Paper on # # # # # LINK http://www.kidney.de/pget.php?&tw=1&pmid=28713180 #FOAvip English Wikipedia <ref>{{Cite pmid|28713180}}</ref> Global observations of magnetospheric high?m poloidal waves during the 22 June 2015 magnetic storm #MMPMID28713180 Le G; Chi PJ; Strangeway RJ; Russell CT; Slavin JA; Takahashi K; Singer HJ; Anderson BJ; Bromund K; Fischer D; Kepko EL; Magnes W; Nakamura R; Plaschke F; Torbert RB Geophys Res Lett 2017[Apr]; 44 (8): 3456-64 PMID28713180show ga We report global observations of high?m poloidal waves during the recovery phase of the 22 June 2015 magnetic storm from a constellation of widely spaced satellites of five missions including Magnetospheric Multiscale (MMS), Van Allen Probes, Time History of Events and Macroscale Interactions during Substorm (THEMIS), Cluster, and Geostationary Operational Environmental Satellites (GOES). The combined observations demonstrate the global spatial extent of storm time poloidal waves. MMS observations confirm high azimuthal wave numbers (m ~ 100). Mode identification indicates the waves are associated with the second harmonic of field line resonances. The wave frequencies exhibit a decreasing trend as L increases, distinguishing them from the single?frequency global poloidal modes normally observed during quiet times. Detailed examination of the instantaneous frequency reveals discrete spatial structures with step?like frequency changes along L. Each discrete L shell has a steady wave frequency and spans about 1 RE, suggesting that there exist a discrete number of drift?bounce resonance regions across L shells during storm times. äGlobal observations of magnetospheric high?m poloidal waves during the(epmc).pdf DeepDyve Pubget Overpricing