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).
Anyone wants to see if there are chances for an auroral display so our site gets lots of traffic. But with higher traffic comes higher server costs. Support our project so we can keep the website online!
|
05:42
May
20
2013
|
Moderately strong M1.77 solar flare |
|
22:36
May
19
2013
|
Weak CME impact Currently we see the effects of the arrival of a Coronal Mass Ejection (CME) at the ACE satellite. The solar wind speed rose with 79.26 km/sec to 455.5 km/sec.
|
|
06:24
May
18
2013
|
G2 - Moderate geomagnetic storm (Kp 6.00) - Observers at high latitudes may see some nice periods of visual aurora. The chances for the Middle latitude is still relatively low. |