Presentation is loading. Please wait.

Presentation is loading. Please wait.

Ovation Pyme Ovation Prime (2010) in Python Liam Kilcommons University of Colorado, Colorado Center for Astrodynamics Research (CCAR), Department.

Published bySylvia Allison Modified over 6 years ago

Similar presentations

Presentation on theme: "Ovation Pyme Ovation Prime (2010) in Python Liam Kilcommons University of Colorado, Colorado Center for Astrodynamics Research (CCAR), Department."— Presentation transcript:

1 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] <

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)
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: /2011SW 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!

Download ppt "Ovation Pyme Ovation Prime (2010) in Python Liam Kilcommons University of Colorado, Colorado Center for Astrodynamics Research (CCAR), Department."

Similar presentations

The Reasons for the Seasons A pre-lab experience….

The Reasons for the Seasons A pre-lab experience….
Abstract Real-time images of Earths space environment from NASAs IMAGE satellite will soon be available on the NOAA Space Environment Center Web site.

Abstract Real-time images of Earths space environment from NASAs IMAGE satellite will soon be available on the NOAA Space Environment Center Web site.
Space Environment Center Service Start to Finish Joe Hirman SEC Lab Review 11-12 July 2000.

Space Environment Center Service Start to Finish Joe Hirman SEC Lab Review July 2000.
10:09:30 AM WP4: Heliosphere and Terrestrial effects Background CME arrival time, L1 solar wind parameters, SEP, magnetopause location, radiation belt.

10:09:30 AM WP4: Heliosphere and Terrestrial effects Background CME arrival time, L1 solar wind parameters, SEP, magnetopause location, radiation belt.
NOAA Non-standard and Test Products for Space Weather AGU – 12/2012 Paper: IN31D-03 William Denig 1 Rodney Viereck 2 1 National Geophysical Data Center.

NOAA Non-standard and Test Products for Space Weather AGU – 12/2012 Paper: IN31D-03 William Denig 1 Rodney Viereck 2 1 National Geophysical Data Center.
4/18 6:08 UT 4/17 6:09 UT Average polar cap flux North cap South cap… South cap South enter (need to modify search so we are here) South exit SAA Kress,

4/18 6:08 UT 4/17 6:09 UT Average polar cap flux North cap South cap… South cap South enter (need to modify search so we are here) South exit SAA Kress,
29 April 2011Viereck: Space Weather Workshop 2011 The Recent Solar Minimum: How Low Was It? What Were The Consequences? Rodney Viereck NOAA Space Weather.

29 April 2011Viereck: Space Weather Workshop 2011 The Recent Solar Minimum: How Low Was It? What Were The Consequences? Rodney Viereck NOAA Space Weather.
The role of solar wind energy flux for transpolar arc luminosity A.Kullen 1, J. A. Cumnock 2,3, and T. Karlsson 2 1 Swedish Institute of Space Physics,

The role of solar wind energy flux for transpolar arc luminosity A.Kullen 1, J. A. Cumnock 2,3, and T. Karlsson 2 1 Swedish Institute of Space Physics,
1 SPACE WEATHER EFFECTS ON SATELLITE DRAG 6 January 2006 Cheryl Huang, Frank A. Marcos and William Burke Space Vehicles Directorate Air Force Research.

1 SPACE WEATHER EFFECTS ON SATELLITE DRAG 6 January 2006 Cheryl Huang, Frank A. Marcos and William Burke Space Vehicles Directorate Air Force Research.
Modelling the Thermosphere-Ionosphere Response to Space Weather Effects: the Problem with the Inputs Alan Aylward, George Millward, Alex Lotinga Atmospheric.

Modelling the Thermosphere-Ionosphere Response to Space Weather Effects: the Problem with the Inputs Alan Aylward, George Millward, Alex Lotinga Atmospheric.
GAII.05 8 July 2003 Data Assimilation Methods for Characterizing Radiation Belt Dynamics E.J. Rigler 1, D.N. Baker 1, D. Vassiliadis 2, R.S. Weigel 1 (1)

GAII.05 8 July 2003 Data Assimilation Methods for Characterizing Radiation Belt Dynamics E.J. Rigler 1, D.N. Baker 1, D. Vassiliadis 2, R.S. Weigel 1 (1)
Peter Wintoft Swedish Institute of Space Physics IUGG, Sapporo, Japan, July 2, 2003 Real time forecasting of geomagnetic indices Peter Wintoft Swedish.

Peter Wintoft Swedish Institute of Space Physics IUGG, Sapporo, Japan, July 2, 2003 Real time forecasting of geomagnetic indices Peter Wintoft Swedish.
Ionospheric Electric Field Variations during Geomagnetic Storms Simulated using CMIT W. Wang 1, A. D. Richmond 1, J. Lei 1, A. G. Burns 1, M. Wiltberger.

Ionospheric Electric Field Variations during Geomagnetic Storms Simulated using CMIT W. Wang 1, A. D. Richmond 1, J. Lei 1, A. G. Burns 1, M. Wiltberger.
SPACE WEATHER FORECASTING II Image courtesy of National Aeronautics and Space Administration (NASA)

SPACE WEATHER FORECASTING II Image courtesy of National Aeronautics and Space Administration (NASA)
~Closing Lesson~ What did you learn from the solar activity? What is the sun made of? What elements are most abundant on the sun? How do you know?

~Closing Lesson~ What did you learn from the solar activity? What is the sun made of? What elements are most abundant on the sun? How do you know?
CISM Advisory Council Meeting 4 March 20031 Ionosphere-Thermosphere Modeling Tim Killeen, Stan Solomon, and the CISM Ionosphere-Thermosphere Team.

CISM Advisory Council Meeting 4 March Ionosphere-Thermosphere Modeling Tim Killeen, Stan Solomon, and the CISM Ionosphere-Thermosphere Team.
What DMSP Data Tell us About the Thermosphere Response to Solar Wind Forcing Delores Knipp CU Aerospace Engineering Sciences and NCAR HAO With Assistance.

What DMSP Data Tell us About the Thermosphere Response to Solar Wind Forcing Delores Knipp CU Aerospace Engineering Sciences and NCAR HAO With Assistance.
Study of the aurora emissions during substorms connected with different solar wind streams I.V. Despirak 1, Zh. V. Dashkevich 1, V. Guineva 2 1. Polar.

Study of the aurora emissions during substorms connected with different solar wind streams I.V. Despirak 1, Zh. V. Dashkevich 1, V. Guineva 2 1. Polar.
New Operational Algorithms for Charged Particle Data from Low-Altitude Polar-Orbiting Satellites J. L. Machol 1,2 *, J.C. Green 1, J.V. Rodriguez 3,4,

New Operational Algorithms for Charged Particle Data from Low-Altitude Polar-Orbiting Satellites J. L. Machol 1,2 *, J.C. Green 1, J.V. Rodriguez 3,4,
Mervyn Freeman British Antarctic Survey

Mervyn Freeman British Antarctic Survey

Similar presentations

Ads by Google