Issued: 2023 Jul 28 1231 UTC
M-class flares expected (probability >=50%)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
28 Jul 2023 | 178 | 005 |
29 Jul 2023 | 175 | 005 |
30 Jul 2023 | 172 | 004 |
Solar flaring activity was moderate during the last 24 hours, with an M1 flare produced by NOAA Active Region (AR) 3388 (magnetic type Beta, Catania group 1) yesterday 22:34 UTC. NOAA AR 3376 (magnetic type Beta, Catania group 86) produced by far the largest number of C-class flares in the last 24 hours with four of them being brighter than C5.0, and one of the brightest, a C7 today 01:09 UTC. NOAA AR 3380 (magnetic type Beta, Catania group 95) produced the third brightest flare of the last 24 hours, a C7 today at 01:46 UTC. NOAA 3387 (magnetic type Alpha, Catania group 3) also produced a C5 flare yesterday at 22:04 UTC. For the next 24 hours the number of C-class flares is expected to drop as NOAA 3376 will rotate out of Earth's view. Nevertheless NOAA AR 3380 has continued to develop and isolated M-class activity is very likely, mostly from this AR, with a small chance of an X-class flare.
No Earth-directed Coronal Mass Ejections (CME) were observed in the last 24 hours. A partial halo CME launched yesterday 21:36 UT is judged to be back-sided.
The Solar Wind (SW) conditions were typical of the slow SW regime during the last 24 hours. The SW speed gradually dropped from 460 km/s to about 380 km/s in the last 24 hours. The total interplanetary magnetic field (Bt) varied between 5 and 7 nT and its North-South component (Bz) ranged between -2 and 4 nT. The interplanetary magnetic field phi angle was directed away from the Sun during the past 24 hours. The SW conditions are expected to remain in the slow SW regime in the next 24 hours.
Geomagnetic conditions were globally at quiet levels (NOAA Kp 1+ to 2) during the past 24 hours. For the same period the conditions were locally at quiet levels (K BEL 1 to 2) with the exception of the 15:00-18:00 period yesterday, when they reached unsettled conditions (K BEL 3). They are expected to remain quiet both locally and globally in the next 24 hours.
The greater than 10 MeV proton flux was at nominal levels over the past 24 hours. However, due to the increased flaring activity on the solar disk, there is a chance of a proton event in the next 24 hours.
The greater than 2 MeV electron flux, as measured by the GOES-16 satellite, was at increased levels during the last 24 hours as a result of the arrival of a HSS at 26 Jul. Nevertheless, the flux remained well below the 1000 pfu alert threshold and is expected to remain below this threshold during the next 24 hours. The 24h electron fluence at nominal levels and is expected to remain so during the next 24 hours.
Today's estimated international sunspot number (ISN): 171, based on 08 stations.
Wolf number Catania | 168 |
10cm solar flux | 165 |
AK Chambon La Forêt | 010 |
AK Wingst | 010 |
Estimated Ap | 008 |
Estimated international sunspot number | 142 - Based on 14 stations |
Day | Begin | Max | End | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types |
---|---|---|---|---|---|---|---|---|---|
27 | 2204 | 2234 | 2305 | S21E68 | M1.7 | SF | --/3388 | VI/1 |
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 |