What is a solar flare

A flare is defined as a sudden, rapid, and intense variation in brightness. A solar flare occurs when magnetic energy that has built up in the solar atmosphere (mostly above sunspots) is suddenly released. Radiation is emitted across virtually the entire electromagnetic spectrum, from radio waves at the long wavelength end, through optical emission to x-rays and gamma rays at the short wavelength end. The amount of energy released is the equivalent of millions of 100-megaton hydrogen bombs exploding at the same time!

Solar Flare

More about solar flares

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There are currently, on the basis of the current data, no chances to see an aurora display on the Middle latitudes
S1 Space radiation storm
At the moment there is a small S1 class space radiation storm active. This happens about 50 times in one solar cycle.

Auroral activity

Live
High latitude (77% chance)
Middle latitude (2% chance)
Low latitude (2% chance)
Today
Minor
Severe
High latitude
30%
55%
Middle latitude
20%
5%

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Raised: 40%

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 60.71 km/sec to 531.5 km/sec.
  • Solar wind speed: 531.5 km/sec and density 4.4 p/cm3
  • IMF Bt (strength): 9.5 nT - Bz -3.8 nT
Weak S1 class Space radiation storm - This happens around 50 times in a solar cycle
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 107.28 km/sec to 558.2 km/sec.
  • Solar wind speed: 558.2 km/sec and density 9.1 p/cm3
  • IMF Bt (strength): 15.4 nT - Bz -14.4 nT

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