Real-time plots auroral activity

Here you'll find plots of the solar wind speed/density and the Interplanetary Magnetic Field (IMF) of the last two hours, these are the first parameters in the predicition of auroral activity. The redder the plots get, the better it is for auroral activity! The Kp plot is a global indicator of the auroral activity on earth in a scale of 0 to 9.

Kiruna Magnetogram

This magnetogram gives you the values measured by the ground station of Kiruna (Sweden, Europa). For middle latitude auroral activity the deflection in the magnetometer data should be more than 1300nT.

EPAM - Electron Proton and Alpha Monitor

EPAM stands for the electron, proton and alpha monitoring and is an instrument in the ACE satellite that measures the electrons and protons that are sent with the solar wind. This is a very useful tool whether the CME is directed towards the Earth and when it will happen.

EPAM - Electron Proton and Alpha Monitor

Real-time solar activity

Sunspot regions

Solar Dynamics Observatory HMI Continuum

Sunspot number: 146 - New regions: 0

Region Number of
sunspots
Class
Magn.
Class
Spot
1744 3 β CAO
1745 8 β CAO
1746 5 β DSO
1747 2 α HRX
1748 23 β - δ - γ FAO
1750 12 β DAI

Solar flare

SDO/EVE Pinhole camera

65% chance for an M-class solar flare
25% chance for an X-class solar flare

Solar flare
Current value
C1.32
Highest value (2h max)
C4.06

Farside

Farside
STEREO Farside

Events on the sun yesterday

Below you'll find an overview of the most worthy solar flares on the sun of the past day, ordered on the date of the event.

No considerable events happened on the sun

There are currently, on the basis of the current data, no chances to see an aurora display on the Middle latitudes
In the past two hours there was a small solar flare with a class of:
C4.06

Auroral activity

Live
High latitude (58% chance)
Middle latitude (0% chance)
Low latitude (0% chance)
Today
Minor
Severe
High latitude
20%
75%
Middle latitude
30%
20%

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Raised: 29%

Latest news

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.
  • Solar wind speed: 455.5 km/sec and density 0.4 p/cm3
  • IMF Bt (strength): 13.4 nT - Bz 3.2 nT
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.
Strong M3.21 solar flare

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