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REAL TIME AURORA OVAL FORECASTING: SVALTRACK II

REAL TIME AURORA OVAL FORECASTING: SVALTRACK II. F. Sigernes 1 , M. Dyrland 1 , P. Brekke 2 , E. K. Gjengedal 3 , S. Chernouss 4 , D.A. Lorentzen 1 , K. Oksavik 1 and C. S. Deehr 5. 1 The University Centre in Svalbard (UNIS), N-9171 Longyearbyen, Norway

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REAL TIME AURORA OVAL FORECASTING: SVALTRACK II

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  1. REAL TIME AURORA OVAL FORECASTING: SVALTRACK II F. Sigernes 1, M. Dyrland 1, P. Brekke 2, E. K. Gjengedal 3, S. Chernouss 4, D.A. Lorentzen 1, K. Oksavik 1 and C. S. Deehr 5 1 The University Centre in Svalbard (UNIS), N-9171 Longyearbyen, Norway 2Norwegian Space Centre, Oslo, Norway 3Storm Weather Center, Bergen, Norway 4Polar Geophysical Institute, Murmansk Region, Apatity, Russia 5 Geophysical Institute, University of Alaska, Fairbanks, USA 37th Annual European Meeting on Atmospheric Studies by Optical Methods, 23-27 August 2010, Valladolid, Spain.

  2. A MATEMATICAL REPRESENTATION OF THE AURORAL OVALS The magnetic input parameter is the AL index – related to the planetary Kp index: Poleward and equatorward boundaries of auroral oval in geomagnetic co-latitude: where amplitudes Aiand phases ai is given by REFERENCES [1] Starkov, G. V., Mathematical model of the auroral boundaries, Geomagnetism and Aeronomy, 34, 3, 331-336, 1994. [2] Starkov, G. V., Statistical dependences between the magnetic activity indices, Geomagnetism and Aeronomy, 34, 1, 101-103, 1994.

  3. COEFFICIENTS Table 1. Expansion coefficients for auroral boundaries by Starkov [1].

  4. GEOGRAPHICAL TRANSFORM Cartesian components: - is the longitudinal difference between the sub-solar point and the magnetic poles at time t (hours). Geographical coordinates: Latitude and longitude:

  5. VISUALIZATION • Includes: • Equatorward boundary of the diffuse aurora • Aurora oval Kp=3 • Magnetic north pole • Field of view aurora observer • Observer location • Moon and Sun information at local site • Position of satellites (Rapideye 1) The oval is visualized with a stand alone 32-bit executable Windows program called SvalTrackII. The program is written in Borland’s Delphi – Pascal and uses a Geographic Information System (GIS) unit called TGlobe. The twilight zone, night- and dayside of the Earth are projected with grades of shade on the Globe as a function of time.

  6. ANIMATION Animated aurora ovals as a function of Kp index [0…8] and time for 24th December 2009

  7. All Sky View Local all sky view of ovals as a function of Kp index [0…8] and time for 24th December 2009 from KHO (78N,16E)

  8. THE +1 HOUR PREDICTED Kp INDEX SOURCE: Space Weather Prediction Centre (SWPC) at the National Oceanic and Atmospheric Administration (NOAA). The Costello Geomagnetic Activity Indexmodel was developed by Kirt Costello at Rice University under support from the US Air Force and Sterling Software, Inc. It is a neural network algorithm that trains on the response of the Kp geomagnetic activity index to solar wind parameters / data. The model returns an one hour prediction in units of Kp. It updates / predicts every 15 minutes. 15 minutes oval update: http://kho.unis.no http://www.swpc.noaa.gov/rpc/costello/costello_latest.html

  9. CONCLUDING REMARK A method to mathematically calculate the size and location of the aurora oval onto a solar illuminated Earth globe is presented as function of estimated Kp index and time. The system may be used as a forecast when the Kp value is estimated from satellite data one hour upstream in the solar wind. PS! The Svaltrack II program is fredware…it cost II beers.

  10. Acknowledgement We wish to thank The National Oceanic and Atmospheric Administration (NOAA) - Space Weather Prediction Centre for allowing us to download the predicted value of the Kp index every 15 minutes. The Research Council of Norway through the project named: Norwegian and Russian Upper Atmosphere Co-operation On Svalbard part 2 # 196173/S30 (NORUSCA2). The Nordic Council of Ministers: Arctic cooperation program # A10162.

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