Välja antud: 2016 Nov 28 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
28 Nov 2016 | 085 | 007 |
29 Nov 2016 | 084 | 006 |
30 Nov 2016 | 083 | 003 |
NOAA 2613, NOAA 2612 and Catania 65 (N05E40) are currently the most prominent sunspot regions on the solar disk. The northern portion of NOAA 2611 was the source of the strongest event of the period, a C1.4 flare at 08:01UT. The region produced also most of the low-level B-class flares, but has now rounded the northwest limb. No earth-directed coronal mass ejections (CMEs) were observed. The greater than 10MeV proton flux was at nominal levels.
Solar flare activity is expected to be at B-class level, with a slight chance on an isolated C-class flare.
Solar wind speed decreased from about 620 km/s to its current values near 450 km/s. Bz fluctuated between -3 nT and +3 nT. The interplanetary magnetic field was mostly directed away from the Sun. Solar wind parameters are expected to further evolve to nominal values as Earth is gradually exiting the high speed stream from the positive coronal hole.
The geomagnetic field was at quiet to unsettled levels, and is expected to remain so.
Today's estimated international sunspot number (ISN): 045, based on 17 stations.
Wolf number Catania | /// |
10cm solar flux | 083 |
AK Chambon La Forêt | 015 |
AK Wingst | 010 |
Estimated Ap | 010 |
Estimated international sunspot number | 031 - Based on 17 stations |
Day | Begin | Max | Lõpp | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
---|---|---|---|---|---|---|---|---|---|---|
Puuduvad |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
Kõik ajad UTC-s
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