Emitido: 2016 May 17 1230 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 17 May 2016 | 102 | 011 |
| 18 May 2016 | 100 | 012 |
| 19 May 2016 | 096 | 013 |
Over the past 24 hours solar activity has been low. The largest flare was a C1.8 class flare. Active Region (AR) 2544 (Macintosh class:Dai; Mag. type:Beta-gamma) produced the largest flare, the C1.8 class flare, peaking at 15:25 UT yesterday. ARs 2544 and 2545 (Cro; Beta) have been the most active regions, producing flares at the B and C class levels. ARs 2542, 2543 and 2545 have all rotated onto the West limb. AR 2544 has exhibited significant flux emergence and cancellation in HMI observations, which may lead to further flares. Solar protons have remained at background levels over the past 24 hours. Solar activity is expected to remain low over the next 24 hours with a high probability of C-class flares and a medium probability of M-class flares. The solar wind speed has remained around 550 km/s over the past 24 hours. The total magnetic field strength has fluctuated around 7 nT. The Bz component fluctuated between -7 and +7 nT. Geomagnetic conditions ranged between Kp index 2-3 (NOAA) and local K index 1-3 (Dourbes) over the past 24 hours. A positive polar coronal hole is currently positioned in the Western hemisphere of the Sun and the resulting high-speed stream (HSS) may enhance solar wind speeds. The CME produced at 15:24 UT on 15-May-2016 may also increase geo-activity at the Earth around 16:30 UT on 18-May-2016.
Today's estimated international sunspot number (ISN): 037, based on 19 stations.
| Wolf number Catania | 106 |
| 10cm solar flux | 102 |
| AK Chambon La Forêt | 022 |
| AK Wingst | /// |
| Estimated Ap | 017 |
| Estimated international sunspot number | 061 - Based on 31 stations |
| Day | Begin | Max | Fin | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
|---|---|---|---|---|---|---|---|---|---|---|
| Ninguno | ||||||||||
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
All times in UTC
< < Ir a la visión general diaria
A lot of people come to SpaceWeatherLive to follow the Solar activity or if there is a chance to see the aurora, but with more traffic comes higher costs to keep the servers online. If you like SpaceWeatherLive and want to support the project you can choose a subscription for an ad-free site or consider a donation. With your help we can keep SpaceWeatherLive online!
| Último evento clase X | 18/01/2026 | X1.9 |
| Último evento clase M | 21/01/2026 | M3.4 |
| Últimas tormentas geomagnéticas | 21/01/2026 | Kp7+ (G3) |
| Días sin manchas | |
|---|---|
| Último día sin manchas | 08/06/2022 |
| Promedio de manchas solares mensuales | |
|---|---|
| diciembre 2025 | 124 +32.2 |
| enero 2026 | 110 -14 |
| Last 30 days | 114.8 +6.7 |