Publié: 2015 Nov 30 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 30 Nov 2015 | 092 | 026 |
| 01 Dec 2015 | 091 | 021 |
| 02 Dec 2015 | 090 | 015 |
Over the past 24 hours solar activity has been low. Only B-class flares have been detected. NOAA Active Regions (AR) 2458 and 2459 have been most active. There is currently a large polar coronal hole at high latitudes and a small transient coronal hole at low latitudes; both have just rotated into the Western hemisphere. No Earth directed CMEs have been detected. A partial halo CME with a speed of 370 +/- 92 km/s was detected by CACTUS on 2015-Nov-29 at 07:24 UT off the South-East limb, the CME is believed to be back-sided and not geo-effective. A second partial halo CME was observed by CACTUS at 02:48 UT on 2015-Nov-30 off the West limb with a speed of 297 +/- 53 km/s, the CME is also believed to be back-sided and will not be geo-effective. Solar activity is expected to remain low over the next 24 hours with the possibility of C-class flares. The solar wind speed has increased over the past 24 hours from 400 km/s to 550 km/s. The total magnetic field strength remained around 10 nT yesterday (2015-Nov-29), and slowly decreased throughout the early hours of this morning. However, it increased to 15 nT between 05:00 and 09:00 UT, and has subsequently been decreasing. The Bz was mainly positive yesterday until around 17:50 UT, when a shock was observed and the field sharply dropped to around -10 nT. The Bz has been mainly negative since then, and dropped to around -15 nT between 05:00 and 09:00 UT this morning before returning to 0 nT. Geomagnetic conditions ranged between Kp index 2-5 (NOAA) and local K index 1-4 (Dourbes) over the past 24 hours. A small low latitude transient coronal hole and large polar coronal hole have just rotated into the Western hemisphere and the resulting high-speed stream (HSS), combined with negative Bz, may increase geo-activity later today.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 048, sur la base de 11 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 096 |
| AK Chambon La Forêt | 019 |
| AK Wingst | 010 |
| Ap estimé | 009 |
| Nombre international de taches solaires estimé | 052 - Basé sur 14 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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