Issued: 2019 Jan 09 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
No forecast
10cm flux | Ap | |
---|---|---|
09 Jan 2019 | 070 | 005 |
10 Jan 2019 | 070 | 004 |
11 Jan 2019 | 070 | 003 |
The solar activity has been quiet over the past 24 hours. The X-ray flux remains below B-level, and the visible solar disc is spotless. Solar activity is expected to remain at low levels.
No Earth directed Coronal Mass Ejection has been observed. The greater than 10 MeV solar protons flux remained at nominal levels over the past 24 hours and is expected to remain so.
The solar wind parameters continued to slowly return toward nominal values. The wind speed decreased from 455 to 395 km/s. Total interplanetary magnetic field strength was below 6 nT. The southward magnetic component remained between -4.5 and 4.7 nT. The solar wind speed is expected to continue to decrease and remain at ambient background and slow solar wind speed regime.
The geomagnetic conditions were quiet and are expected to remain quiet during the following next 24-hour period.
Today's estimated international sunspot number (ISN): 000, based on 18 stations.
Wolf number Catania | 000 |
10cm solar flux | 071 |
AK Chambon La Forêt | 010 |
AK Wingst | 006 |
Estimated Ap | 005 |
Estimated international sunspot number | 000 - Based on 22 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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