Issued: 2016 Jun 21 1232 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
21 Jun 2016 | 084 | 013 |
22 Jun 2016 | 083 | 010 |
23 Jun 2016 | 083 | 007 |
Solar activity was low with X-ray flux remaining below C Level. All the regions on the visible disk are fairly simple, NOAA AR 2558 can produce C-class flares. Two partial halo CMEs occurred in past 24h. The first one on June 20 at 16:36 UT (first seen by LASCO/C2) was backsided, the second one at 04:36 UT today was very slow and originated from NOAA AR 2553 close to the western solar limb (W70), no geomagnetic consequences are expected. Solar wind speed is at 400 km/s. The interplanetary magnetic field intensity at 4 nT. Geomagnetic conditions have been quiet. Active conditions can be expected for the next 48 h, due to a high speed stream from a coronal hole.
Today's estimated international sunspot number (ISN): 023, based on 12 stations.
Wolf number Catania | 037 |
10cm solar flux | 084 |
AK Chambon La Forêt | 009 |
AK Wingst | 005 |
Estimated Ap | 004 |
Estimated international sunspot number | 035 - Based on 20 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
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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
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Last M-flare | 2025/04/08 | M1.5 |
Last geomagnetic storm | 2025/04/06 | Kp5 (G1) |
Spotless days | |
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Last spotless day | 2022/06/08 |
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