Emitido: 2016 Apr 06 1240 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 06 Apr 2016 | 084 | 010 |
| 07 Apr 2016 | 083 | 009 |
| 08 Apr 2016 | 084 | 008 |
Over the past 24 hours solar activity has slightly increased with respect to the previous 2 days. A slow Coronal Mass Ejection (CME) has been detected yesterday at 13:36 UT, which evolved from a small filament eruption on the disk adjacent to AR 2528. It has a small probability to hit the Earth around 09-Apr-2016. The largest flare was a C1.1 class flare, which peaked at 10:11 UT this morning. There are two ARs currently on the solar disk; AR 2528 (Macintosh class:Gro; Mag.type:Beta-Gamma) and AR 2527. AR 2526 is going to move over the solar limb in the next 24 hours, while one returning region will appear at the East limb within next 24 hrs. 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 some probability of C-class flares. The solar wind speed has increased slightly over the past 24 hours, fluctuating between 350 to 450 km/s over the past 24 hours. The total magnetic field strength remained stable with the magnitude varying between 8 and 10 nT. The Bz component remained around 0 nT, varying between +7 and -6 nT. Geomagnetic conditions ranged between Kp index 1-3 (NOAA) and local K index 1-3 (Dourbes) over the past 24 hours. There is currently a small transient coronal hole on disk, stretching from the South-East to center disk. Geomagnetic activity is expected to remain low over the next 2 days. However, in 3 days the level of geomagnetic activity has some chances to increase due to a small CME that occurred yesterday, the CME is related to a filament eruption that occurred around 13.00UT. We can also expect to encounter a high speed stream in approximately 3 days time.
Today's estimated international sunspot number (ISN): 020, based on 19 stations.
| Wolf number Catania | 040 |
| 10cm solar flux | 083 |
| AK Chambon La Forêt | 011 |
| AK Wingst | 007 |
| Estimated Ap | 006 |
| Estimated international sunspot number | 032 - Based on 30 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 | 08/12/2025 | X1.1 |
| Último evento clase M | 21/12/2025 | M1.3 |
| Últimas tormentas geomagnéticas | 22/12/2025 | Kp5 (G1) |
| Días sin manchas | |
|---|---|
| Último día sin manchas | 08/06/2022 |
| Promedio de manchas solares mensuales | |
|---|---|
| noviembre 2025 | 91.8 -22.8 |
| diciembre 2025 | 115.2 +23.4 |
| Last 30 days | 109.1 +22.6 |