Issued: 2019 Dec 01 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
01 Dec 2019 | 070 | 003 |
02 Dec 2019 | 070 | 003 |
03 Dec 2019 | 070 | 005 |
Solar activity was at very low levels. The visible solar disk was spotless. No earth-directed coronal mass ejections (CMEs) have been observed in available coronagraphic imagery. The greater than 10 MeV proton flux was at nominal values. A weak extension from the southern polar coronal hole has transited the central meridian.
Solar activity is expected to remain at very low levels.
Solar wind speed was on a generally declining trend, from about 400 km/s at the beginning to near 360 km/s by the end of the period (ACE). The interplanetary magnetic field (phi angle) was directed towards the Sun (negative sector). Bz varied between -5 and +3 nT, most of the time being close to 0 nT. Geomagnetic activity was at quiet levels.
Geomagnetic activity is expected to remain at mostly quiet levels, an unsettled interval not excluded on 3 or 4 December if the weak CH wind stream affects the earth environment.
Today's estimated international sunspot number (ISN): 000, based on 08 stations.
Wolf number Catania | /// |
10cm solar flux | 070 |
AK Chambon La Forêt | 006 |
AK Wingst | 004 |
Estimated Ap | 003 |
Estimated international sunspot number | /// - Based on /// stations |
Day | Begin | Max | End | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
---|---|---|---|---|---|---|---|---|---|---|
None |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
All times in UTC
Current data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future
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Spotless days | |
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Last spotless day | 2022/06/08 |
Monthly mean Sunspot Number | |
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Last 30 days | 137.9 +0.4 |