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10.1002/2015JA021778 http://scihub22266oqcxt.onion/10.1002/2015JA021778 C5076489!5076489!27830111     free     free     free Deprecated: Implicit conversion from float 227.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 227.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 227.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 227.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 227.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 227.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 227.6 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 261.2 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 261.2 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 261.2 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534 Deprecated: Implicit conversion from float 261.2 to int loses precision in C:\Inetpub\vhosts\kidney.de\httpdocs\pget.php on line 534       J+Geophys+Res+Space+Phys 2016 ; 121 (3): 2171-84 Nephropedia Template TP {{tp|p=27830111|t=2016. Intense energetic electron flux enhancements in Mercury s magnetosphere: An integrated view with high?resolution observations from MESSENGER |pdf=|usr=}}{{27830111}} gab.com Text Intense energetic electron flux enhancements in Mercury s magnetosphere: An integrated view with high resolution observations from MESSENGER JO: J Geophys Res Space Phys http://www.kidney.de/pget.php?&tw=1&pmid=27830111 #FOAvip The MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) mission to Mercury has provided a wealth of new data about energetic particle phenomena. With observations from MESSENGER's Energetic Particle Spectrometer, as well as data arising from energetic electrons recorded by the X?Ray Spectrometer and Gamma?Ray and Neutron Spectrometer (GRNS) instruments, recent work greatly extends our record of the acceleration, transport, and loss of energetic electrons at Mercury. The combined data sets include measurements from a few keV up to several hundred keV in electron kinetic energy and have permitted relatively good spatial and temporal resolution for many events. We focus here on the detailed nature of energetic electron bursts measured by the GRNS system, and we place these events in the context of solar wind and magnetospheric forcing at Mercury. Our examination of data at high temporal resolution (10?ms) during the period March 2013 through October 2014 supports strongly the view that energetic electrons are accelerated in the near?tail region of Mercury's magnetosphere and are subsequently ?injected? onto closed magnetic field lines on the planetary nightside. The electrons populate the plasma sheet and drift rapidly eastward toward the dawn and prenoon sectors, at times executing multiple complete drifts around the planet to form ?quasi?trapped? populations. Twit Text FOAVip Intense energetic electron flux enhancements in Mercury s magnetosphere: An integrated view with high resolution observations from MESSENGER ????J Geophys Res Space Phys http://www.kidney.de/pget.php?&tw=1&pmid=27830111 #FOAvip Twit Text # Free Paper on # # # # # LINK http://www.kidney.de/pget.php?&tw=1&pmid=27830111 #FOAvip English Wikipedia <ref>{{Cite pmid|27830111}}</ref> Intense energetic electron flux enhancements in Mercury s magnetosphere: An integrated view with high?resolution observations from MESSENGER #MMPMID27830111 Baker DN; Dewey RM; Lawrence DJ; Goldsten JO; Peplowski PN; Korth H; Slavin JA; Krimigis SM; Anderson BJ; Ho GC; McNutt RL; Raines JM; Schriver D; Solomon SC J Geophys Res Space Phys 2016[Mar]; 121 (3): 2171-84 PMID27830111show ga The MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) mission to Mercury has provided a wealth of new data about energetic particle phenomena. With observations from MESSENGER's Energetic Particle Spectrometer, as well as data arising from energetic electrons recorded by the X?Ray Spectrometer and Gamma?Ray and Neutron Spectrometer (GRNS) instruments, recent work greatly extends our record of the acceleration, transport, and loss of energetic electrons at Mercury. The combined data sets include measurements from a few keV up to several hundred keV in electron kinetic energy and have permitted relatively good spatial and temporal resolution for many events. We focus here on the detailed nature of energetic electron bursts measured by the GRNS system, and we place these events in the context of solar wind and magnetospheric forcing at Mercury. Our examination of data at high temporal resolution (10?ms) during the period March 2013 through October 2014 supports strongly the view that energetic electrons are accelerated in the near?tail region of Mercury's magnetosphere and are subsequently ?injected? onto closed magnetic field lines on the planetary nightside. The electrons populate the plasma sheet and drift rapidly eastward toward the dawn and prenoon sectors, at times executing multiple complete drifts around the planet to form ?quasi?trapped? populations. äIntense energetic electron flux enhancements in Mercury s magnetospher(epmc).pdf DeepDyve Pubget Overpricing