Publié: 2014 Dec 04 1221 UTC
Eruptive (C-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 04 Dec 2014 | 153 | 010 |
| 05 Dec 2014 | 149 | 010 |
| 06 Dec 2014 | 145 | 011 |
Majority of the low-level C-class flares and the M1.3 flare (peaking at 08:10 UT) observed this morning, originated from the Catania sunspot group 24 (NOAA AR 2222). The SDO/AIA data do not show on-disc signatures of the possibly associated CME, so we conclude that the M1.3 flare was most probably one of the numerous confined flares which originated from the Catania sunspot group 24 (NOAA AR 2222). Catania sunspot groups 18 and 24 (NOAA ARs 2217 and 2222) maintain beta-gamma configuration of the photospheric magnetic field and are expected to be the sources of C-class flares and possibly also an isolated M-class flare. No Earth directed CMEs were observed during last 24 hours. At the midday of December 3 the solar wind speed started to increase until it reached the value of about 500 km/s which is also observed at the present time. Concurrently with the increase of the solar wind speed, the interplanetary magnetic field magnitude increased to the value of about 10nT. This slightly elevated value of the interplanetary magnetic field magnitude is still present. The fast solar wind originating from the large polar coronal hole with the extent to the low latitudes (up to about S40) might be expected at the Earth in the morning of December 6. We expect quiet to unsettled geomagnetic conditions to continue in the next 24 hours.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 067, sur la base de 03 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 154 |
| AK Chambon La Forêt | 014 |
| AK Wingst | 008 |
| Ap estimé | 008 |
| Nombre international de taches solaires estimé | 088 - Basé sur 11 stations |
| Jour | Commencer | Max | Fin | Loc | Force | OP | 10cm | Catania/NOAA | Types de sursaut radio |
|---|---|---|---|---|---|---|---|---|---|
| 04 | 0800 | 0810 | 0821 | S24W27 | M1.3 | 1N | 24/2222 |
Données fournies par le Solar Influences Data analysis Center© - SIDC - Traité par SpaceWeatherLive
Toutes les heures sont indiquées en UTC
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!
| Dernière classe X | 08/12/2025 | X1.1 |
| Dernière classe M | 31/12/2025 | M7.11 |
| Dernier orage géomagnétique | 02/01/2026 | Kp5 (G1) |
| Jours sans taches solaires | |
|---|---|
| Dernier jour sans taches solaires | 08/06/2022 |
| Nombre mensuel moyen de taches solaires | |
|---|---|
| décembre 2025 | 124 +32.2 |
| janvier 2026 | 122 -2 |
| 30 derniers jours | 111.1 +8.3 |