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10.1002/2015GL066376 http://scihub22266oqcxt.onion/10.1002/2015GL066376 C4777921!4777921!27019537     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 Deprecated: Implicit conversion from float 211.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534       Geophys+Res+Lett 2015 ; 42 (23): 10113-9 Nephropedia Template TP {{tp|p=27019537|t=2015. Acceleration and loss of relativistic electrons during small geomagnetic storms |pdf=|usr=}}{{27019537}} gab.com Text Acceleration and loss of relativistic electrons during small geomagnetic storms JO: Geophys Res Lett http://www.kidney.de/pget.php?&tw=1&pmid=27019537 #FOAvip Past studies of radiation belt relativistic electrons have favored active storm time periods, while the effects of small geomagnetic storms (Dst > ?50 nT) have not been statistically characterized. In this timely study, given the current weak solar cycle, we identify 342 small storms from 1989 through 2000 and quantify the corresponding change in relativistic electron flux at geosynchronous orbit. Surprisingly, small storms can be equally as effective as large storms at enhancing and depleting fluxes. Slight differences exist, as small storms are 10% less likely to result in flux enhancement and 10% more likely to result in flux depletion than large storms. Nevertheless, it is clear that neither acceleration nor loss mechanisms scale with storm drivers as would be expected. Small geomagnetic storms play a significant role in radiation belt relativistic electron dynamics and provide opportunities to gain new insights into the complex balance of acceleration and loss processes. Twit Text FOAVip Acceleration and loss of relativistic electrons during small geomagnetic storms ????Geophys Res Lett http://www.kidney.de/pget.php?&tw=1&pmid=27019537 #FOAvip Twit Text # Free Paper on # # # # # LINK http://www.kidney.de/pget.php?&tw=1&pmid=27019537 #FOAvip English Wikipedia <ref>{{Cite pmid|27019537}}</ref> Acceleration and loss of relativistic electrons during small geomagnetic storms #MMPMID27019537 Anderson BR; Millan RM; Reeves GD; Friedel RHW Geophys Res Lett 2015[Dec]; 42 (23): 10113-9 PMID27019537show ga Past studies of radiation belt relativistic electrons have favored active storm time periods, while the effects of small geomagnetic storms (Dst > ?50 nT) have not been statistically characterized. In this timely study, given the current weak solar cycle, we identify 342 small storms from 1989 through 2000 and quantify the corresponding change in relativistic electron flux at geosynchronous orbit. Surprisingly, small storms can be equally as effective as large storms at enhancing and depleting fluxes. Slight differences exist, as small storms are 10% less likely to result in flux enhancement and 10% more likely to result in flux depletion than large storms. Nevertheless, it is clear that neither acceleration nor loss mechanisms scale with storm drivers as would be expected. Small geomagnetic storms play a significant role in radiation belt relativistic electron dynamics and provide opportunities to gain new insights into the complex balance of acceleration and loss processes. äAcceleration and loss of relativistic electrons during small geomagnet(epmc).pdf DeepDyve Pubget Overpricing