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OvationPyme Diffuse Auroral Energy Flux [mW/m^2] <-------

Ovation Pyme Ovation Prime (2010) in Python Liam Kilcommons University of Colorado, Colorado Center for Astrodynamics Research (CCAR) , Department of Aerospace Engineering Sciences (AES). OvationPyme Diffuse Auroral Energy Flux [mW/m^2] <-------. What is Ovation Prime?.

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OvationPyme Diffuse Auroral Energy Flux [mW/m^2] <-------

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  1. Ovation PymeOvation Prime (2010) in PythonLiam KilcommonsUniversity of Colorado, Colorado Center for Astrodynamics Research (CCAR), Department of Aerospace Engineering Sciences (AES) OvationPyme Diffuse Auroral Energy Flux [mW/m^2] <-------

  2. What is Ovation Prime? • Model of high latitude electron precipitation made using DMSP SSJ data • Total energy flux, number flux, average electron energy for three types of electron precipitation & proton precipitation • Driven by solar wind coupling function based on NASA Omniweb data

  3. Ovation Prime 2010 (NOAA Version) https://sourceforge.net/projects/ovation-prime/ • Parent of Ovation Pyme • Written in IDL • See this paper for details on performance Machol, J. L., J. C. Green, R. J. Redmon, R. A. Viereck, and P. T. Newell (2012), Evaluation of OVATION Prime as a forecast model for visible aurorae, Space Weather, 10, S03005, doi:10.1029/2011SW000746. Ovation Pyme is a direct rewrite of the NOAA IDL code in Python, with a few extra features • There are other versions of Ovation: • JHU APL’s Ovations ( 2010, SM, 2013 ) • 2013 is better than 2010 for strong storm-time

  4. Extra Feature: Ionospheric Conductance Empirical Model for Solar Conductance (Brekke & Moen) Robinson Formula For Auroral Conductance

  5. Thanks! https://github.com/lkilcommons/OvationPyme Contributions, bug reports, and comments are very welcome!

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