Issued: 2019 Jan 15 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
15 Jan 2019 | 070 | 007 |
16 Jan 2019 | 070 | 017 |
17 Jan 2019 | 070 | 013 |
Solar X-ray flux remained below B level throughout the period. There are no active regions on disk and X-ray flux is expected to continue to be below C level.
No earth directed CMEs have been recorded.
The proton flux levels were at background values and are expected to remain so.
Solar wind was close to nominal with Solar wind speed recovering from around 400 km/s at the start of the period to a minimum of 330 km/s, while presently around 360 km/s. Total magnetic field was in the 2-8.5 nT range with Bz variable. The magnetic field phi angle was in the negative sector. Solar wind may become somewhat enhanced again tomorrow under the possible influence of the coronal hole that passed central meridian midnight January 12/13.
Geomagnetic conditions were quiet to unsettled (local K Dourbes and NOAA Kp 1-3). Quiet to unsettled conditions are expected over the next days with a possibility for an isolated active period.
Today's estimated international sunspot number (ISN): 000, based on 14 stations.
Wolf number Catania | /// |
10cm solar flux | 070 |
AK Chambon La Forêt | 013 |
AK Wingst | 010 |
Estimated Ap | 007 |
Estimated international sunspot number | 000 - Based on 30 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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Active geomagnetic conditions (Kp4) Threshold Reached: 22:47 UTC
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Active geomagnetic conditions (Kp4) Threshold Reached: 01:41 UTC
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