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Predictions of auroral activity since 1994 have been based on the repetitive nature of solar disturbances during approximately four years of minimum solar activity. Solar activity began to increase in 1998, however, and stronger effects are felt due to sporadic solar activity, which cannot be predicted on the longer term. Therefore, we have changed our forecast format in keeping with more active and less predictable solar activity. The predictions are now mainly based on interpretations of satellite observations of active structures on the sun and of the solar wind between the sun and the earth. We expect this situation to prevail until around 2003.
The Aurora Forecast is produced by the Geophysical Institute Auroral Forecast Team of S. Akasofu, C. Deehr, D. Lummerzheim, and W. Sun. Questions about the aurora may be directed to the GI Information Office at info@gi.alaska.edu. The Aurora Forecast web site is based on the original design by Don Rice and is produced by the Digital Design Center at the Geophysical Institute. Additional notes on interpreting these forecasts are available. You may also wish to examine current geomagnetic storminess at the HAARP site , as well as links to Aurora sites worldwide. |
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