Emitido: 2021 Mar 09 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 09 Mar 2021 | 080 | 011 |
| 10 Mar 2021 | 080 | 012 |
| 11 Mar 2021 | 079 | 007 |
The X-ray flux remained below C-level. Active region NOAA 2806 is turning behind the limb. A new region, Catania group 78 is rotating to the disk in the NE. X-ray flux is expected to remain below C-level.
No Earth-directed Coronal Mass Ejections (CMEs) have been observed in coronagraph data.
The greater than 10 MeV proton flux was at nominal levels over the past 24 hours and is expected to remain so for the next 24 hours. The greater than 2 MeV electron flux peaked over the 1000 pfu event threshold during its diurnal maximum and is expected do so again today. The 24h electron fluence reached moderate levels and is expected to remain on those levels considering the enhanced solar wind conditions.
A low latitude corona hole of negative polarity in the southern hemisphere is expected to start crossing the central meridian today. Its effects to the solar wind conditions are expected after the noon of the 12th March.
Solar wind showed a slow decline of the enhanced solar wind conditions. Solar wind speed is around 450 km/s and is expected to slowly decline further. The magnetic field strength is below 5 nT and is expected to remain weak. The magnetic field was directed away from the Sun. Solar wind conditions are expected to further decay slowly over the next couple of days. The corona hole crossing the solar meridian today is expected to effect the solar wind conditions in approximately 3 days. By that time a boundary crossing is expected to occur. The magnetic field strength to increase significantly.
Geomagnetic conditions were quiet to unsettled (both NOAA Kp and local K Dourbes had values 0-3). They are expected to remain quiet to unsettled with a general decaying trend. An increase is expected beginning in the 12 March, as today's coronal hole crossing is expected to affect the geomagnetic conditions.
Today's estimated international sunspot number (ISN): 022, based on 09 stations.
| Wolf number Catania | /// |
| 10cm solar flux | 080 |
| AK Chambon La Forêt | 010 |
| AK Wingst | 008 |
| Estimated Ap | 006 |
| Estimated international sunspot number | 013 - Based on 24 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 | 14/01/2026 | M1.6 |
| Últimas tormentas geomagnéticas | 11/01/2026 | Kp5+ (G1) |
| Días sin manchas | |
|---|---|
| Último día sin manchas | 08/06/2022 |
| Promedio de manchas solares mensuales | |
|---|---|
| diciembre 2025 | 124 +32.2 |
| enero 2026 | 93.1 -30.9 |
| Last 30 days | 98.3 -7.4 |