| GOES 15 X-Ray Events 1-8A | |||
| Cur | 12/1148 | C1.0 | Ratio 0.008 |
| Beg |
12/0857
|
C1.0
| |
| Max |
12/0903
|
C1.6
| Int 1.5e-03 J m-2 |
| End |
12/0914
|
C1.3
| |
The GOES X-ray flux plot contains 1 minute averages of solar X-rays in the 1-8 Angstrom (0.1-0.8 nm) and 0.5-4.0 Angstrom (0.05-0.4 nm) passbands. Data from the SWPC Primary GOES X-ray satellite is shown. As of Feb 2008, no Secondary GOES X-ray satellite data is available. Some data dropouts will occur during satellite eclipses.During the spring and fall, GOES satellites experience eclipses in which the Earth or moon blocks the X-ray instrument view to the sun for a short period every day. Eclipse season lasts for about 45 to 60 days and ranges from minutes to just over an hour. At these times there is a gap in the XRS signal shown.Other plots of interest: 3-day GOES 5-min X-rays; SWPC Real-time Monitors.SWPC X-ray alerts are issued at the M5 (5x10E-5 Watts/m2) level, 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.
Se ha producido una llamarada solar de clase C 8.0 de larga duración,
en una nueva mancha solar que tipifican como S2407 (S28E73) que esta apareciendo por el limbo sureste.
