Publié: 2015 Jun 29 1230 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 29 Jun 2015 | 095 | 011 |
| 30 Jun 2015 | 094 | 006 |
| 01 Jul 2015 | 093 | 007 |
Solar activity has been low, NOAA AR 2373 has just rotated into view and has the potential to produce several flares, it has already produced 3 C-class flares in the past 24 hours, the largest being a C1.9 flare peaking at 17:14 UT on 2015-06-28. The previously active AR 2371 has rotated over the West limb, but produced the largest magnitude flare in the past 24 hours, a C2.2 flare peaking at 00:36 UT on 2015-06-29. Other recurrent active regions are rotating into view now and may increase solar activity in the coming hours. Proton levels are still declining and are now below 5 pfu. The solar wind speed has slightly decreased over the past 24 hours, and has varied between 350 km/s to 480 km/s. The total magnetic field has been around 6 nT with small variations ranging from 4 to 8 nT, and the Bz component has fluctuated from positive to negative, between +6 and -5 nT over the past 24 hours. Geomagnetic conditions ranged between Kp index 2-3 (NOAA) and local K index 1-4 over the past 24 hours. There were no significant CMEs over the past 24 hours.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 034, sur la base de 17 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | /// |
| AK Chambon La Forêt | 017 |
| AK Wingst | 016 |
| Ap estimé | 015 |
| Nombre international de taches solaires estimé | 023 - Basé sur 25 stations |
| Jour | Commencer | Max | Fin | Loc | Force | OP | 10cm | Catania/NOAA | Types de sursaut radio | |
|---|---|---|---|---|---|---|---|---|---|---|
| Aucun | ||||||||||
Données fournies par le Solar Influences Data analysis Center© - SIDC - Traité par SpaceWeatherLive
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