Issued: 2017 Nov 09 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
09 Nov 2017 | 068 | 022 |
10 Nov 2017 | 068 | 019 |
11 Nov 2017 | 068 | 006 |
The solar activity is quiet as the solar disc remains spotless; no flares and no active regions have been recorded in past 24 h on the disc. The X-ray flux is expected to remain below C level.
No Earth directed Coronal Mass Ejections have been observed and the solar protons flux remained at background levels over the past 24 hours.
The Earth remained in the fast solar wind with a speed of about 600-650 km/s. On Nov 09 early morning the solar wind started to decrease slowly to reached the speed of 550 km/s. The interplanetary magnetic field magnitude has also slowly decreased from 7 nT to below 5 nT. The Bz component was fluctuating between -7 and 7 nT being mainly negative and is currently around -5 nT. The solar wind speed is expected to continue to decrease until it reaches its nominal level by tomorrow.
Due to the fast solar wind and the Bz component of the interplanetary magnetic field being manly southward, unsettle to disturb geomagnetic conditions were observed with local K Dourbes 2-5 and NOAA Kp 3-5. The geomagnetic conditions are expected to remain disturb as long as the Earth remains in the solar wind flow associated with the high speed stream coming from the coronal hole (that has crossed the central meridian on Nov 4). Minor geomagnetic storms cannot be excluded, especially if Bz component remains negative for long period of time.
Today's estimated international sunspot number (ISN): 000, based on 16 stations.
Wolf number Catania | 000 |
10cm solar flux | 068 |
AK Chambon La Forêt | 053 |
AK Wingst | 041 |
Estimated Ap | 049 |
Estimated international sunspot number | 000 - Based on 11 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 high possibility for aurora to appear at the following high latitude regions in the near future
Rovaniemi, Sodankylä, UtsjokiCurrent data suggests there is a moderate possibility for aurora to appear at the following high latitude regions in the near future
TórshavnCurrent data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future
KuopioCurrent data suggests there is a slight possibility for aurora to appear at the following middle latitude regions in the near future
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The OVATION model predicts the Hemispheric Power Index to reach 75GW at 21:49 UTC
Minor G1 geomagnetic storm (Kp5) Threshold Reached: 13:07 UTC
The OVATION model predicts the Hemispheric Power Index to reach 75GW at 13:21 UTC
Minor G1 geomagnetic storm (Kp5) Threshold Reached: 23:59 UTC
Minor G1 geomagnetic storm (Kp5) Threshold Reached: 20:02 UTC
Last X-flare | 2025/03/28 | X1.1 |
Last M-flare | 2025/04/01 | M2.5 |
Last geomagnetic storm | 2025/03/27 | Kp5 (G1) |
Spotless days | |
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Last spotless day | 2022/06/08 |
Monthly mean Sunspot Number | |
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March 2025 | 134.2 -20.4 |
April 2025 | 143 +8.8 |
Last 30 days | 130.4 -16.1 |