The Interplanetary Electron Model (IEM)
Taylor, BO, Underwood, CI, Vacanti, G and Maddox, E (2011) The Interplanetary Electron Model (IEM) In: NSREC 2011, 2011-07-25 - 2010-07-29, Las Vegas, NV, USA.
Available under License : See the attached licence file.
Plain Text (licence)
A new Interplanetary electron environment model based on statistical analyses of historical datasets is presented. The model reports generates confidence limits for solar electron fluences in a similar fashion to existing Solar proton models, as well as peak event fluxes and fluences. Electrons of Jovian origin are also modeled based on simplified diffusive transport equations to provide predicted fluxes for locations within the ecliptic plane.
|Item Type:||Conference or Workshop Item (Conference Paper)|
|Divisions :||Faculty of Engineering and Physical Sciences > Electronic Engineering|
|Date :||18 November 2011|
|Identification Number :||https://doi.org/10.1109/TNS.2011.2171718|
|Additional Information :||
Copyright 2008 IEEE. Personal use of this material is permitted. However, permission to reprint/republish this material for advertising or promotional purposes or for creating new collective works for resale or redistribution to servers or lists, or to reuse any copyrighted component of this work in other works must be obtained from the IEEE.
|Depositing User :||Symplectic Elements|
|Date Deposited :||08 Feb 2012 10:28|
|Last Modified :||23 Sep 2013 18:54|
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