Issued: 2020 Jul 12 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
12 Jul 2020 | 068 | 005 |
13 Jul 2020 | 068 | 009 |
14 Jul 2020 | 068 | 014 |
Solar activity was at very low levels and is expected to remain so. The solar disk was spotless. Old active region NOAA 2766 was the source of two A2 flares peaking on 11 July at resp. 10:20UT and 20:50UT. Coronal dimming and weak EIT waves were observed, but the associated CMEs were very faint.
No earth-directed coronal mass ejections (CMEs) were observed in available coronagraphic imagery.
The greater than 10 MeV proton flux and the greater than 2 MeV electron flux were at nominal levels during the last 24 hours and are expected to remain so.
Solar wind speed was on a slightly declining trend from initial values near 330 km/s to 290 km/s by the end of the period (DSCOVR and ACE). Bz varied between -3 and +1 nT. The direction of the interplanetary magnetic field (phi angle) was mostly directed away from the Sun (positive sector).
Geomagnetic activity was at quiet levels. Geomagnetic conditions are expected to be mostly quiet, with unsettled intervals possible on 12-13 July from coronal hole wind stream effects, and on 14 July from a glancing blow from the 09 July CME. An isolated active interval is not excluded.
Today's estimated international sunspot number (ISN): 000, based on 28 stations.
Wolf number Catania | /// |
10cm solar flux | 069 |
AK Chambon La Forêt | 005 |
AK Wingst | 003 |
Estimated Ap | 002 |
Estimated international sunspot number | 000 - 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 high possibility for aurora to appear at the following high latitude regions in the near future
ReykjavikCurrent data suggests there is a moderate possibility for aurora to appear at the following high latitude regions in the near future
TórshavnCurrent data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future
KuopioCurrent data suggests there is a slight possibility for aurora to appear at the following middle latitude regions in the near future
TampereA 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!
Minor G1 geomagnetic storm (Kp5) Threshold Reached: 23:17 UTC
The OVATION model predicts the Hemispheric Power Index to reach 75GW at 21:49 UTC
Minor G1 geomagnetic storm (Kp5) Threshold Reached: 13:07 UTC
The OVATION model predicts the Hemispheric Power Index to reach 75GW at 13:21 UTC
Minor G1 geomagnetic storm (Kp5) Threshold Reached: 23:59 UTC
Last X-flare | 2025/03/28 | X1.1 |
Last M-flare | 2025/04/01 | M2.5 |
Last geomagnetic storm | 2025/03/27 | Kp5 (G1) |
Spotless days | |
---|---|
Last spotless day | 2022/06/08 |
Monthly mean Sunspot Number | |
---|---|
March 2025 | 134.2 -20.4 |
April 2025 | 143 +8.8 |
Last 30 days | 129.8 -16.3 |