Issued: 2015 Oct 18 1230 UTC
M-class flares expected (probability >=50%)
Minor storm expected (A>=30 or K=5)
Quiet
10cm flux | Ap | |
---|---|---|
18 Oct 2015 | 119 | 031 |
19 Oct 2015 | 122 | 021 |
20 Oct 2015 | 125 | 021 |
Solar flaring intensified due to a new region currently rounding the southeast solar limb. This new sunspot group produced 6 C-class flares and 2 M1 flares, the latter peaking resp. at 20:23UT and 20:42UT. NOAA 2434 produced 3 low-level C-class flares, originating from the small delta north of the main spot. NOAA 2435 and NOAA 2436 produced one C1 flare each, while NOAA 2431 was quiet. No earth-directed coronal mass ejections have been observed.
Further M-class flaring is likely, in particular from NOAA 2434 and the new region at the southeast solar limb.
Around 22:00UT, solar wind speed started a gradual rise from around 350 km/s to its current values between 400 and 450 km/s. Bz was mostly negative, with persistent values around -5 nT between 15-21UT and a strong -11 nT during the 06-09UT interval. The direction of the interplanetary magnetic field (IMF) varied wildly. In response to the persistently negative Bz, Kp reached active levels during the 18-21UT and 06-09UT intervals. Kp and local K were at minor storming levels during the last interval of the period. A negative equatorial CH may affect the geomagnetic environment late around 21 October.
Mostly quiet to active geomagnetic conditions are expected, with a chance on another minor storming episode from the moderate speed stream.
Today's estimated international sunspot number (ISN): 068, based on 11 stations.
Wolf number Catania | /// |
10cm solar flux | 117 |
AK Chambon La Forêt | 019 |
AK Wingst | 013 |
Estimated Ap | 012 |
Estimated international sunspot number | 071 - Based on 11 stations |
Day | Begin | Max | End | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types |
---|---|---|---|---|---|---|---|---|---|
17 | 2009 | 2023 | 2028 | ---- | M1.1 | --/---- | |||
17 | 2035 | 2042 | 2046 | ---- | M1.5 | --/---- |
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
Whitehorse, YT, Yellowknife, NTA 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!
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 | 2025/04/08 | M1.5 |
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 |