Emesso: 2014 Jun 08 1323 UTC
Eruptive (C-class flares expected, probability >=50%)
Minor storm expected (A>=30 or K=5)
Quiet
10cm flux | Ap | |
---|---|---|
08 Jun 2014 | 140 | 031 |
09 Jun 2014 | 140 | 009 |
10 Jun 2014 | 140 | 006 |
A single C1.9 flare was observed at 10:02 UT on 8 June from a region behind the east limb. Catania sunspot groups 69 and 76 (resp NOAA ARs 2080 and 2085) have grown in size and number of sunspots. A halo CME was observed in LASCO/C2 and STEREO A & B COR2 coronagraphic imagery with first measurement in LASCO/C2 at 3:24 UT on 8 June. The CME is mainly propagating to the west of the Sun-Earth line, but further analysis is needed to determine whether this CME has an Earth-bound component. C-class flaring activity is expected for the next 48 hours, with an increasing chance for M-class flaring, especially from Catania groups 69 and 76. ACE observed a shock in the solar wind speed at 16:10 UT on 7 June, with simultaneous increases in speed, density, temperature and magnitude of IMF. The magnitude of the IMF went first to 15 nT, reached a maximum of 29 nT at 6:55 UT and has now dropped to about 15 nT again. The Bz-component was fluctuating between negative and positive values. Local K-index at Dourbes went to K=5 and estimated NOAA Kp even reached K=6 on the UT morning of 8 June. The solar wind speed increased from 340 km/s to 550 km/s. The shock is probably related to the arrival of a glancing blow of the 4 June CME. Geomagnetic storm conditions are expected to continue in the next few hours and will return then to quiet to unsettled conditions on 9 June.
Today's estimated international sunspot number (ISN): 098, based on 19 stations.
Wolf number Catania | /// |
10cm solar flux | 137 |
AK Chambon La Forêt | 029 |
AK Wingst | 018 |
Estimated Ap | 017 |
Estimated international sunspot number | 098 - Based on 24 stations |
Day | Begin | Max | Fine | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
---|---|---|---|---|---|---|---|---|---|---|
Nessuna |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
Tutti gli orari in UTC
<< Vai alla pagina della panoramica giornaliera
Molte persone vengono su SpaceWeatherLive per seguire l'attività del Sole o sapere se ci sia la possibilità di vedere l'aurora, ma a maggior traffico corrispondono costi maggiori. Considerate una donazione se vi piace SpaceWeatherLive così che possiamo mantenere online il sito web!
Ultimo brillamento X | 2025/03/28 | X1.1 |
Ultimo brillamento M | 2025/04/05 | M1.0 |
Ultima tempesta geomagnetica | 2025/04/06 | Kp5 (G1) |
Giorni senza macchie | |
---|---|
Ultimo giorno senza macchie | 2022/06/08 |
Media mensile Numero di Macchie Solari | |
---|---|
marzo 2025 | 134.2 -20.4 |
aprile 2025 | 148.7 +14.5 |
Ultimi 30 giorni | 132.7 -9.9 |