Issued: 2017 Sep 26 1322 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
26 Sep 2017 | 092 | 004 |
27 Sep 2017 | 094 | 016 |
28 Sep 2017 | 096 | 010 |
Solar activity slightly increased over the past 24 hours. Two numbered active regions (AR) regions on the visible disk AR 2681 (Cso; Beta), AR 2682 (Hax; Alpha), produced multiple B-class flares. The newly- numbered AR 2683 (Hkx; Apha) produced the largest C1.8 flare which peaked at 02:34 UT today (26-Sep-2017). One eruptive dimming has been observed at the solar disk center at 15:23 UT yesterday, an associated CME departed mostly toward the East with the projected speed around 490 km/s. More coronograph imagery is needed before conclusion can be made. One filament erupted from the east solar limb at 22:20 UT yesterday; the associated slow CME is not expected to be geoeffective. Solar activity is expected to remain low over the next 24 hours with a probability of C-class flares. Solar wind parameters returned to nominal levels during the past 24 hours. Solar wind speed decreased from around 400 km/s to 315 km/s. Total field strength remained below 3.5 nT, while Bz component varied between 2.5 and -2.5 nT. Solar wind parameters are expected remain at near background levels today (26-Sep-2017). Solar wind variations can increase tomorrow (27 September, 2017) due to the influence of the transequatorial positive polarity CH HSS. Geomagnetic conditions ranged between Kp index 0-2 (NOAA) and local K index 0-2 (Dourbes) over the past 24 hours. The geomagnetic field is expected to be at quiet levels today and may reach a minor storm level tomorrow (27-Sep-2017).
Today's estimated international sunspot number (ISN): 040, based on 18 stations.
Wolf number Catania | 039 |
10cm solar flux | 090 |
AK Chambon La Forêt | 006 |
AK Wingst | 005 |
Estimated Ap | 004 |
Estimated international sunspot number | 039 - Based on 29 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
Arkhangelsk, VorkutaA 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 M1.08 flare
Minor R1 radio blackout in progress (≥M1 - current: M1.04)
Active geomagnetic conditions (Kp4) Threshold Reached: 22:47 UTC
The OVATION model predicts the Hemispheric Power Index to reach 50GW at 21:37 UTC
Active geomagnetic conditions (Kp4) Threshold Reached: 01:41 UTC
Last X-flare | 2025/03/28 | X1.1 |
Last M-flare | 2025/04/11 | M1.0 |
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 | 141.4 +7.2 |
Last 30 days | 137.9 +0.4 |