Emitido: 2021 Mar 24 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 24 Mar 2021 | 079 | 007 |
| 25 Mar 2021 | 082 | 007 |
| 26 Mar 2021 | 082 | 007 |
Solar activity was at very low levels in the past 24 hours. NOAA AR 2811 and Catania group 81 produced only minor B-class flares. A new small active region that rotated into view has been numbered by NOAA as AR 2812 (alpha magnetic field configuration). Solar activity is expected to remain at low levels, with a small chance of a C-class flare.
A Coronal Mass Ejection (CME) was observed on 22 March, 01:10 UT. It has an Earth-directed component and its speed is estimated to 250-300 km/s. It is expected to reach Earth on 26 March.
An equatorial negative polarity coronal hole crossed the central meridian, its associated high speed stream will arrive at the Earth in about 3 days.
The greater than 10 MeV proton flux was below 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 exceeded the 1000 pfu threshold in the past 24 hours and is expected to remain elevated in the next 24 hours. The 24h electron fluence was at moderate levels in the last 24 hours and is expected to remain at moderate levels in the next 24 hours.
The solar wind speed decreased from 500 km/s to 420 km/s. The interplanetary magnetic field magnitude varied between 1 and 5 nT. Bz was between 3 and -4 nT. The magnetic field phi angle showed alternating polarity. Slow solar wind conditions are expected in the next 24 hours.
Geomagnetic conditions were quiet to unsettled, Kp varied between 2 and 3 and local K Dourbes between 1 and 3 over the past 24 hours. The CME observed on 20 March could still arrive today and cause at most active conditions (otherwise mostly quiet conditions expected).
Today's estimated international sunspot number (ISN): 027, based on 16 stations.
| Wolf number Catania | /// |
| 10cm solar flux | 079 |
| AK Chambon La Forêt | 019 |
| AK Wingst | 013 |
| Estimated Ap | 012 |
| Estimated international sunspot number | 025 - Based on 20 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 | 11/01/2026 | M3.3 |
| 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 | 97.4 -9.1 |