Datum verslag: 2025 Jul 20 1231 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| 10cm flux | Ap | |
|---|---|---|
| 20 Jul 2025 | 155 | 008 |
| 21 Jul 2025 | 150 | 006 |
| 22 Jul 2025 | 145 | 005 |
Solar flaring activity was low over the past 24 hours, with seven C-class flares identified. SIDC Sunspot Group 559 (NOAA Active Region [AR] 4143, Beta-Gamma magnetic configuration) produced three of those flares. SIDC Sunspot Group 562 (NOAA AR 4136, Beta-Gamma magnetic configuration) and SIDC Sunspot Group 564 (NOAA AR 4149, Beta magnetic configuration) produced two flares each. The brightest flare of the past 24 hours was SIDC flare 4922, a double-peaked C7 flare with the highest peak on 20 Jul at 07:41 UTC. More C-class flaring activity is expected in the next 24 hours, with a chance of an isolated M-class flare.
No Earth-directed Coronal Mass Ejections (CME) were observed in the last 24 hours.
SIDC Coronal Hole (CH) 116 with negative polarity started crossing the central solar meridian during the past 24 hours. Due to its elongated and irregular shape it is not expected to produce a very fast High Speed Stream (HSS). In any case, any effects on the Earth's atmosphere from this CH crossing are expected to register on 23 Jul.
The Solar Wind (SW) conditions returned to a slow SW regime during the past 24 hours. The SW speed dropped from 520 to 400 km/s, while the interplanetary magnetic field (B) ranged between 3 and 6 nT, and its North-South component (Bz) fluctuated between -5 and 5 nT. A similar pattern is expected for the next 24 hours.
The geomagnetic conditions registered globally quiet levels (NOAA Kp 1- to 2+) and locally quiet to unsettled levels (BEL 2 to 3). They are expected to remain at those levels during the next 24 hours.
The greater than 10 MeV proton flux, as measured by the GOES-19 satellite, was at background levels over the past 24 hours and is expected to remain so in the next 24 hours.
The greater than 2 MeV electron flux, as measured by GOES 19, was above the 1000 pfu alert threshold during the past 24 hours. It is expected to remain above the alert threshold in the next 24 hours. The 24-hour electron fluence increased from moderate to high levels on 20 Jul at 05:00 UTC. It is expected to remain at high levels in the next 24 hours.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 157, gebaseerd op 12 stations.
| Wolfgetal Catania | /// |
| 10cm zonneflux | 153 |
| AK Chambon La Forêt | 014 |
| AK Wingst | 010 |
| Geschatte Ap | 009 |
| Geschat internationaal zonnevlekkengetal | 159 - Gebaseerd op 19 stations |
| Dag | Start | Max | Einde | Locatie | Sterkte | OP | 10cm | Catania/NOAA | Soorten radio-uitbarstingen | |
|---|---|---|---|---|---|---|---|---|---|---|
| Geen | ||||||||||
Aangeboden door het Solar Influences Data Analysis Center© - SIDC - Verwerkt door SpaceWeatherLive
Alle tijden in UTC
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