GOES 12 GOES 10
Cur 0248 M1.4 Ratio 0.114 0248 M1.5 Ratio 0.102
Beg 0109 M1.2 0109 M1.1
Max 0129 X3.0 Int 3.93e-01 J m-2 0130 X2.7 Int 3.62e-01 J m-2
End 0144 X1.5 0145 X1.3

This GOES X-ray flux plot contains 1 minute averages of solar X-ray output in the 1-8 Angstrom (0.1-0.8 nm) and 0.5-4.0 Angstrom (0.05-0.4 nm) passbands. Data from both operational GOES satellites are included. Some data dropouts will occur during satellite eclipses. SEC alerts are issued at the M5 (5x10E-5 Watts/m2) and X1 (1x10E-4 Watts/m2) levels, based upon 1-minute data. Large X-ray bursts cause short wave fades for HF propagation paths through the sunlit hemisphere. Some large flares are accompanied by strong solar radio bursts that may interfere with satellite downlinks.


CME aimed to East, SOHO image.

CME


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