Issued: 2023 Aug 23 1231 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
23 Aug 2023 | 151 | 007 |
24 Aug 2023 | 153 | 007 |
25 Aug 2023 | 155 | 007 |
There are eight active regions visible on the disk, a new region rotated over the east limb (NOAA AR 3415). They all have simple alpha or beta magnetic field configuration. An M1.1 flare occurred on 22 August, with peak at 23:04 UTC, from NOAA AR 3405. C-class flares are expected and M-class flares are possible in the next 24 hours.
A wide CME (angular width around 80 degrees) erupted to the west, first seen at 19:00 UTC on 22 August by LASCO-C2. The source region of this CME is slightly backsided and thus the CME will not arrive to the Earth. About 1 hour later, a faint CME could be seen erupting towards the southeast, related to dimmings seen on EUV around NOAA ARs 3405 and 3411 (this activity is also related to the M1.1 flare from NOAA AR 3405). Due to the location of the dimmings (close to disk center), a possible arrival to the Earth of this faint CME cannot be discarded (on 26 August). Later on, one more faint CME erupted from NOAA AR 3404, in the vicinity of the previous eruption and first seen at 02:00 UTC by LASCO-C2. This last CME will most likely not affect Earth (although more data will be investigated as it becomes available).
The Earth is inside a slow solar wind stream, with speed around 430 km/s and an interplanetary magnetic field around 5 nT. The interplanetary magnetic field orientation was predominantly in the negative sector (field directed towards the Sun). Similar conditions can be expected in the next 24 hours.
During the last 24 hours the geomagnetic conditions were quiet (NOAA KP 1-2, K Bel 1-2). Similar conditions can be expected for the next 24 hours.
Over the past 24 hours the greater than 10 MeV GOES proton flux was at nominal levels and is expected to remain so over the next 24 hours.
The greater than 2 MeV electron flux remained below the 1000 pfu threshold as measured by GOES 16. It is expected to remain so in the next 24 hours. The 24 hour electron fluence was at normal levels and is expected to remain so.
Today's estimated international sunspot number (ISN): 105, based on 23 stations.
Wolf number Catania | 127 |
10cm solar flux | 151 |
AK Chambon La Forêt | 010 |
AK Wingst | 008 |
Estimated Ap | 008 |
Estimated international sunspot number | 119 - Based on 28 stations |
Day | Begin | Max | End | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types |
---|---|---|---|---|---|---|---|---|---|
22 | 2235 | 2304 | 2338 | N11W29 | M1.1 | SF | 27/3405 | CTM/2VI/2 |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
All times in UTC
A 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!
Last X-flare | 2025/03/28 | X1.1 |
Last M-flare | 2025/04/01 | M5.6 |
Last geomagnetic storm | 2025/03/27 | Kp5 (G1) |
Spotless days | |
---|---|
Last spotless day | 2022/06/08 |
Monthly mean Sunspot Number | |
---|---|
February 2025 | 154.6 +17.6 |
Last 30 days | 128.5 -22.7 |