Odnotowany: 2021 Jul 01 1254 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| strumień 10cm | Ap | |
|---|---|---|
| 01 Jul 2021 | 095 | 018 |
| 02 Jul 2021 | 095 | 021 |
| 03 Jul 2021 | 093 | 019 |
Two C flares were observed from NOAA region 2835, of which a C3.6 flare peaking at 18:15UT. NOAA region 2835 continued to grow and continues to show mixed polarity in the intermediate spots and the leading part. It is classified as beta- gamma-delta magnetic configuration. Bipolar region NOAA 2836 and unipolar region NOAA 2837 are both in decay. Flaring at C level is likely (mostly from NOAA 2835) over the next 24 hours, with also a chance for a possible M flare.
No new Earth directed CMEs have been recorded in coronagraph data.
The greater than 10 MeV proton flux was at nominal levels over the past 24 hours and is expected to remain so for the next 24 hours. The greater than 2 MeV electron flux was below the 1000 pfu event threshold. The 24h electron fluence was at normal levels and electron fluence is expected to initially remain at normal levels during the next days, but may then start rising if enhanced solar wind conditions persist.
Solar wind conditions displayed the expected increase in Solar wind speed due to the forecasted high speed stream. Solar wind speed reached 520km/s by 21UT and has been around 500km/s since then. The magnetic field remained elevated and reached peaks over 13nT with also Bz seeing periods of consistently negative values down to -10nT, though Bz has been positive more recently since 1UT. The persistent increased magnetic field and the variations in magnetic field orientation seem to indicate that the high speed stream is carrying some transients along. This is possibly allready the June 27 CME that was expected later today. Solar wind conditions are expected to remain enhanced as the transients are passing. Later, on July 3, there is again a possible CME arrival from the June 29 CME.
Geomagnetic conditions were quiet to active (local K Dourbes 2-4 and NOAA Kp 1-4). Geomagnetic conditions are expected to be unsettled with isolated active periods possible.
Dzisiejsza szacunkowa międzynarodowa liczba plam na Słońcu (ISN): 053, na podstawie 18 stacji.
| Liczba Wolfa z Katanii | /// |
| Fale radiowe 10,7 cm | 094 |
| AK Chambon La Forêt | 025 |
| AK Wingst | 017 |
| Szacunkowa Ap | 016 |
| Szacowana międzynarodowa liczba plam słonecznych | 056 - Na podstawie stacji 30 |
| 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 | 2026/02/04 | X4.21 |
| Ostatnie rozbłyski klasy M | 2026/02/16 | M2.4 |
| Ostatnia burza geomagnetyczna | 2026/02/22 | Kp5+ (G1) |
| Dni bez plam słonecznych | |
|---|---|
| Ostatnie 365 dni | 1 Dzień |
| 2026 | 1 Dzień (2%) |
| Aktualny odcinek | 2 Dni |
| Średnia miesięczna liczba plam słonecznych | |
|---|---|
| stycznia 2026 | 112.6 -11.4 |
| lutego 2026 | 86.1 -26.5 |
| Ostatnie 30 dni | 95.9 -24.7 |