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.