Chart originally from http://sec.noaa.gov/rt_plots/xray_1m.html
| GOES 12 | GOES 10 |
| Cur | 2124 | X1.0 | Ratio 0.128 | 2124 | X1.0 | Ratio 0.121 | ||
| Beg | 2037 | C9.5 | 2037 | C9.0 | ||||
| Max | 2049 | X 11 | Int 9.11e-01 J m-2 | 2049 | X 10 | Int 8.74e-01 J m-2 | ||
| End | 2100 | X5.4 | 2101 | X4.6 |
Chart originally from http://sec.noaa.gov/rt_plots/xray_1m.html
| GOES 12 | GOES 10 |
| Cur | 2124 | X1.0 | Ratio 0.128 | 2124 | X1.0 | Ratio 0.121 | ||
| Beg | 2037 | C9.5 | 2037 | C9.0 | ||||
| Max | 2049 | X 11 | Int 9.11e-01 J m-2 | 2049 | X 10 | Int 8.74e-01 J m-2 | ||
| End | 2100 | X5.4 | 2101 | X4.6 |
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.
