Publié: 2014 Oct 30 1248 UTC
Active (M-class flares expected, probability >=50%)
Active conditions expected (A>=20 or K=4)
Warning condition (activity levels expected to increase, but no numeric forecast given)
| Flux de 10 cm | Ap | |
|---|---|---|
| 30 Oct 2014 | 130 | 010 |
| 31 Oct 2014 | 120 | 006 |
| 01 Nov 2014 | 120 | 005 |
Seven M-class flares and six C-class flares were counted since the last bulletin. An M3.5 flare was the largest flare, peaking at 1:35 UT, originating from Catania sunspot group 88 (NOAA AR 2192). Catania group 88 is currently located at the west limb and although it is difficult to determine it's characteristics, the region seems to have shrinked. All other regions on the front side of the solar disk were relatively stable. Catania group 88 is still capable to produce large flares, mainly at the M-level, with a minor chance for another X-flare. We retain the warning condition for a proton event. No Earth-directed CMEs were observed in coronagraphic imagery. The solar wind speed observed by ACE is low at around 350 km/s. The interplanetary magnetic field has a magnitude of about 5 nT. A sector boundary crossing is observed at about 08:00 UT on October 30 as the phi angle changed from a mostly positive to negative orientation. Mostly quiet geomagnetic conditions are expected, with a chance for an isolated time slot of active conditions (K=4).
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 080, sur la base de 11 stations.
| Nombre de Wolf, observé par Catania | 128 |
| Flux solaire à 10 cm | 150 |
| AK Chambon La Forêt | 013 |
| AK Wingst | 008 |
| Ap estimé | 008 |
| Nombre international de taches solaires estimé | 070 - Basé sur 12 stations |
| Jour | Commencer | Max | Fin | Loc | Force | OP | 10cm | Catania/NOAA | Types de sursaut radio |
|---|---|---|---|---|---|---|---|---|---|
| 29 | 1424 | 1433 | 1451 | S16W81 | M1.4 | SF | 88/2192 | III/2 | |
| 29 | 1606 | 1620 | 1633 | ---- | M1.0 | 88/2192 | |||
| 29 | 1847 | 1850 | 1852 | ---- | M1.3 | 88/2192 | |||
| 29 | 2118 | 2122 | 2125 | ---- | M2.3 | --/---- | |||
| 30 | 0034 | 0037 | 0040 | ---- | M1.3 | --/---- | |||
| 30 | 0119 | 0135 | 0156 | ---- | M3.5 | --/---- | III/1 | ||
| 30 | 0417 | 0428 | 0436 | S16E62 | M1.2 | SF | --/---- |
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 | 18/01/2026 | X1.9 |
| Dernière classe M | 21/01/2026 | M3.4 |
| Dernier orage géomagnétique | 20/01/2026 | Kp8 (G4) |
| 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 | 107.3 -16.8 |
| 30 derniers jours | 111.9 +4 |