Publié: 2013 Jun 30 1259 UTC
Eruptive (C-class flares expected, probability >=50%)
Minor storm expected (A>=30 or K=5)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 30 Jun 2013 | 102 | 021 |
| 01 Jul 2013 | 105 | 030 |
| 02 Jul 2013 | 107 | 007 |
Solar activity has been eruptive during the past 24 hours, featuring two low C flares from NOAA 11778 and NOAA 11781. More C flares are possible within the next 48 hours, with a slight chance for an M flare, especially from NOAA AR 11778, 11780 and 11781. Solar wind density increased around 5:00 UT on June 29, while wind speed and temperature began to rise, marking the arrival of the expected coronal hole high speed stream. Meanwhile, solar wind speed has increased from about 360 km/s to 500 km/s. In the past 24 hours, geomagnetic activity has been at quiet to active levels (K Dourbes between 1 and 4; NOAA Kp between 2 and 4). A rise to minor storm levels is possible on June 30 and the first half of July 1st, due to an expected glancing blow from the CME of 02:00 UT on June 28. Quiet to active levels are likely in the second half of July 1st, and a return to quiet levels is expected on July 2nd.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 050, sur la base de 14 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 100 |
| AK Chambon La Forêt | 037 |
| AK Wingst | 035 |
| Ap estimé | 048 |
| Nombre international de taches solaires estimé | 045 - Basé sur 22 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
Toutes les heures sont indiquées en UTC
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