Issued: 2016 Nov 06 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Minor storm expected (A>=30 or K=5)
Quiet
10cm flux | Ap | |
---|---|---|
06 Nov 2016 | 077 | 006 |
07 Nov 2016 | 076 | 007 |
08 Nov 2016 | 075 | 033 |
Solar activity was very low in the past 24 hours. No flares were observed. A partial halo CME is visible in SoHO/LASCO C2 images from 00:00 UT onwards on November 5. The ejection is mostly directed towards the North-East and has an angular extent of 200 degrees. The speed is measured to be at most 400 km/s. The origin of the event is most likely be related to the filament eruption around 00:00 UT November 5, in the North-Western quadrant. Solar Protons have remained at background levels over the past 24 hours. Solar activity is expected to remain low over the next 24 hours with a low probability of C-class flares. Variations of the solar wind parameters were very low. Solar wind speed decreased from about 365 km/s to its current values near 315 km/s. Total Interplanetary Magnetic Field (IMF) strength fluctuated between 4.7 nT and 5.5 nT, while Bz fluctuated between +3.2 nT and -3.1 nT. As the result the geomagnetic conditions have been low in the past 24 hours, (K Dourbes between 0 and 3; NOAA Kp between 0 and 2). The geomagnetic environment is expected to continue at low levels today (November 6) and tomorrow (November 7). However, late on the day three (November 8) or the day four (November 9, early in the morning) Earth may experience the passage of the flanks of the CME. Given the low speed and the direction of the CME effects are estimated not to be very strong with possibly minor up to moderate geomagnetic storms.
Today's estimated international sunspot number (ISN): 024, based on 10 stations.
Wolf number Catania | /// |
10cm solar flux | 077 |
AK Chambon La Forêt | 005 |
AK Wingst | 002 |
Estimated Ap | 001 |
Estimated international sunspot number | 026 - Based on 18 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 moderate possibility for aurora to appear at the following middle latitude regions in the near future
SurgutCurrent data suggests there is a slight possibility for aurora to appear at the following middle latitude regions in the near future
Kazan, Perm, Yakutsk, YekaterinburgA lot of people come to SpaceWeatherLive to follow the Sun's activity or if there is aurora to be seen, but with more traffic comes higher server costs. Consider a donation if you enjoy SpaceWeatherLive so we can keep the website online!
Moderate G2 geomagnetic storm (Kp6) Threshold Reached: 16:34 UTC
Minor G1 geomagnetic storm (Kp5) Threshold Reached: 15:20 UTC
Strong G3 geomagnetic storm (Kp7) Threshold Reached: 14:18 UTC
Moderate G2 geomagnetic storm (Kp6) Threshold Reached: 13:21 UTC
The OVATION model predicts the Hemispheric Power Index to reach 125GW at 14:01 UTC
Last X-flare | 2025/03/28 | X1.1 |
Last M-flare | 2025/04/15 | M1.2 |
Last geomagnetic storm | 2025/04/15 | Kp6+ (G2) |
Spotless days | |
---|---|
Last spotless day | 2022/06/08 |
Monthly mean Sunspot Number | |
---|---|
March 2025 | 134.2 -20.4 |
April 2025 | 124.1 -10.1 |
Last 30 days | 124.7 -16.6 |