This model gives a forecast of the intensity of the auroral oval and is based on the solar wind conditions and the Interplanetary Magnetic Field. The map shows the intensity and the location of the auroral oval for the time given in the bottom of the map. The forecast is based on the current solar wind conditions and the average time for the solar wind to propagate from the ACE satellite at the L1 Lagrange point to Earth. The red line indicates how far away viewers on the ground might see the aurora, assuming good viewing conditions.
These plots shows you the current extent of the auroral oval in the northern hemisphere (left) and the southern hemisphere (right), extrapolated from the measurements taken during the most recent pass of the NOAA POES satellite.
The red arrow points to the direction of the sun (daylight side).
|Predicted Kp max||3|
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04:48 Oct 30 2014
|Moderate M1.25 solar flare from sunspot region 12192|
01:54 Oct 30 2014
|Strong M3.56 solar flare from sunspot region 12192|
00:54 Oct 30 2014
|Moderate M1.36 solar flare from sunspot region 12192|
|Last geomagnetic storm:||2014/10/20||Kp5 (G1)|