Существующий: 2017 May 17 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 17 May 2017 | 074 | 017 |
| 18 May 2017 | 074 | 024 |
| 19 May 2017 | 074 | 010 |
In the past 24 hours, no C flares were observed. Very low solar activity (no C flares) is expected in the next 24 hours. Solar wind speed measured by DSCOVR decreased from about 550 to 470 km/s in the past 24 hours. The magnitude of the Interplanetary Magnetic Field (IMF) varied between about 2 and 6 nT. Solar wind speed is expected to decrease further within the next 24 hours. On May 17 or early on May 18, a glancing blow from the partial halo CME of May 13 may enhance solar wind conditions again. Quiet to unsettled geomagnetic conditions (K Dourbes between 1 and 3; NOAA Kp between 1 and 3) were registered in the past 24 hours. Quiet to unsettled levels are expected on May 17, 18 and the first half of May 19, with a chance for active geomagnetic levels (K Dourbes = 4) and a slight chance for minor geomagnetic storm intervals (K Dourbes = 5) on May 17 and 18. Active to minor storm conditions are possible late on May 19, as the high speed stream of a negative equatorial coronal hole is expected to arrive at Earth.
Today's estimated international sunspot number (ISN): 012, based on 22 stations.
| Wolf number Catania | 027 |
| 10cm solar flux | 072 |
| AK Chambon La Forêt | 013 |
| AK Wingst | 010 |
| Estimated Ap | 010 |
| Estimated international sunspot number | 024 - Based on 26 stations |
| Day | Begin | Max | Конец | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
|---|---|---|---|---|---|---|---|---|---|---|
| Нет | ||||||||||
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
Все время в UTC
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