Odnotowany: 2021 Aug 07 1232 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| strumień 10cm | Ap | |
|---|---|---|
| 07 Aug 2021 | 075 | 018 |
| 08 Aug 2021 | 076 | 015 |
| 09 Aug 2021 | 076 | 007 |
Regions NOAA 2850, 2851 and 2852 are all plages now. Region 2850 produced a few low B flares in the past 24 hours. The chance for a C flare in the next 24 hours is estimated at 25%, especially from region 2850 and the yet unnumbered region at the NE limb.
No Earth-directed Coronal Mass Ejections (CMEs) were observed in available coronagraphic imagery.
The greater than 10 MeV proton flux was at nominal levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours. The greater than 2 MeV electron flux was at nominal levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours. The greater than 2 MeV electron fluence was at nominal levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours.
Around 04:30 UT on August 7, The Interplanetary Magnetic Field (IMF) as registered by DSCOVR changed orientation to away from the Sun, its magnitude increased from about 6 to 13 nT (current values are around 8 nT), and the solar wind speed started rising from about 320 km/s to current values of about 410 km/s. At around the same time, a drop in solar wind density was observed. This probably marks the arrival of the predicted high speed stream associated with the positive polarity northern polar crown coronal hole. Bz was below -5 nT most of the time between 14:00 UT on August 6 and 04:30 UT on August 7 and between 09:00 UT and 11:00 UT on August 7, with a minimal value of about -9 nT. Enhanced solar wind conditions are possible on August 7 and 8, and a return to nominal solar wind conditions is expected on August 9.
Quiet to unsettled geomagnetic conditions (K Dourbes between 2 and 3; NOAA Kp between 2 and 3) were registered in the past 24 hours. Active intervals (K Dourbes = 4) are possible on August 7 and 8 due to the arrival of an expected high speed stream, with a chance for minor storm intervals (K Dourbes = 5). A return to quiet to unsettled geomagnetic levels (K Dourbes < 4) is expected on August 9.
Dzisiejsza szacunkowa międzynarodowa liczba plam na Słońcu (ISN): 000, na podstawie 22 stacji.
| Liczba Wolfa z Katanii | 012 |
| Fale radiowe 10,7 cm | 074 |
| AK Chambon La Forêt | 019 |
| AK Wingst | 008 |
| Szacunkowa Ap | 008 |
| Szacowana międzynarodowa liczba plam słonecznych | 008 - Na podstawie stacji 29 |
| Dzień | Początek | Maksymalnie | Koniec | Lokalizacja | Siła | OP | 10cm | Katania/NOAA | Typy impulsów radiowych | |
|---|---|---|---|---|---|---|---|---|---|---|
| Żaden | ||||||||||
Dostarczone przez Centrum Analizy Danych Wpływów Słonecznych© - SIDC - Przetworzone przez SpaceWeatherLive
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| Ostatnie rozbłyski klasy X | 2025/12/08 | X1.1 |
| Ostatnie rozbłyski klasy M | 2025/12/31 | M7.11 |
| Ostatnia burza geomagnetyczna | 2026/01/10 | Kp6 (G2) |
| Dni bez plam słonecznych | |
|---|---|
| Ostatni dzień bez plamy słonecznej | 2022/06/08 |
| Średnia miesięczna liczba plam słonecznych | |
|---|---|
| grudnia 2025 | 124 +32.2 |
| stycznia 2026 | 102.5 -21.5 |
| Ostatnie 30 dni | 100.5 -9 |