Issued: 2015 Oct 04 1234 UTC
C-class flares expected, (probability >=50%)
Minor storm expected (A>=30 or K=5)
Warning condition (activity levels expected to increase, but no numeric forecast given)
10cm flux | Ap | |
---|---|---|
04 Oct 2015 | 090 | 016 |
05 Oct 2015 | 080 | 017 |
06 Oct 2015 | 080 | 007 |
During the past period, there were only three active regions on the solar disk. Four lower C-class flares and one M1.0 (peaking at 2:41 UT on October 4) flare were observed. The M1 flare originated from NOAA 2422, though being almost completely behind the West limb. NOAA 2427 now is a beta-gamma region, though it did not produce any significant flares the past 24 hours. Flaring activity at the C-level is expected. An extended equatorial positive polarity coronal hole has reached the central meridian and will be geo-effective within about 3 days.
Solar wind observations show a slight increase in speed (up to 500 km/s) and temperature from 15 UT October 4 on. The interplanetary magnetic field magnitude was maximally around 10 nT, with a mainly negative Bz component. Solar wind is expected to remain slightly disturbed and possibly indicate the arrival of a glancing blow related to the September 30 CME later today. Geomagnetic conditions were unsettled at the local level (Dourbes K=3) and active (NOAA Kp=4 at 3-6 UT) to even minor storm (NOAA Kp=5 at 9 UT) levels at the planetary level. Geomagnetic activity could be at to active or minor storm conditions during the next 24 hours.
Today's estimated international sunspot number (ISN): 021, based on 10 stations.
Wolf number Catania | /// |
10cm solar flux | 097 |
AK Chambon La Forêt | 020 |
AK Wingst | 008 |
Estimated Ap | 009 |
Estimated international sunspot number | 046 - Based on 12 stations |
Day | Begin | Max | End | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types |
---|---|---|---|---|---|---|---|---|---|
04 | 0234 | 0241 | 0248 | ---- | M1.0 | --/2422 |
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
Iqaluit, NUA 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 M1.66 flare from sunspot region 4055
Minor R1 radio blackout in progress (≥M1 - current: M1.01)
The OVATION model predicts the Hemispheric Power Index to reach 50GW at 21:39 UTC
Moderate M3.24 flare from sunspot region 4055
Minor R1 radio blackout in progress (≥M1 - current: M1.07)
Last X-flare | 2025/03/28 | X1.1 |
Last M-flare | 2025/04/13 | M1.6 |
Last geomagnetic storm | 2025/04/06 | Kp5 (G1) |
Spotless days | |
---|---|
Last spotless day | 2022/06/08 |
Monthly mean Sunspot Number | |
---|---|
March 2025 | 134.2 -20.4 |
April 2025 | 136.4 +2.2 |
Last 30 days | 134.2 -8.9 |