Odnotowany: 2020 Jul 30 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| strumień 10cm | Ap | |
|---|---|---|
| 30 Jul 2020 | 073 | 003 |
| 31 Jul 2020 | 074 | 003 |
| 01 Aug 2020 | 074 | 005 |
The solar activity remained at very low levels over the past 24 hours. The two unipolar sunspot regions visible on the disc, namely Catania 37/N0AA-AR 2767, classified as alpha/Hsx, and N0AA-AR 2768, classified as alpha/Axx, remained stable and did not produce any significant flares. The observed X-ray flux remained below B-class level. The solar activity is expected to remain at low levels over the next 24 hours.
No Earth directed Coronal Mass Ejections (CMEs) were observed in the available coronagraph imagery.
The greater than 10 MeV proton flux was at background levels over the past 24 hours and is expected to remain so for the next 24 hours. Over the past 24 hours the greater than 2 MeV electron flux fluctuated between moderate and background levels remaining well below the active threshold. This behaviour is expected to persist over the next 24 hours.
Over the past 24 hours the solar wind conditions remained mostly quiet, based on data from ACE and DSCOVR. The total interplanetary magnetic field varied between 1 nT and 7 nT. The north-south Bz component fluctuated between -7 nT and 4 nT, with highest absolute value at 04:00 UTC today. The Phi angle was rapidly flipping between long-term intervals with positive and negative orientation.
In the past 24 hours the solar wind speed remained relatively stable with small variations between 315 km/s and 380 km/s. The solar wind conditions are expected to remain quiet over the next 24 hours.
A positive polarity northern coronal hole (CH 64) which resided in the north-east quadrant for several days has now crossed the central meridian facing the Earth. An associated HSS emanating from this coronal hole is expected to reach the Earth within the next 3 to 5 days.
A small-amplitude rarefaction wave arrived at Earth around 18 UTC yesterday resulting in a 2 hour period of locally unsettled conditions with K Dourbes index equal to 3. The global geomagnetic conditions remained quiet with maximum Kp-NOAA index equal to 2. The geomagnetic conditions are expected to remain mostly quiet over the next 24 hours.
Dzisiejsza szacunkowa międzynarodowa liczba plam na Słońcu (ISN): 020, na podstawie 22 stacji.
| Liczba Wolfa z Katanii | /// |
| Fale radiowe 10,7 cm | 073 |
| AK Chambon La Forêt | 008 |
| AK Wingst | 006 |
| Szacunkowa Ap | 004 |
| Szacowana międzynarodowa liczba plam słonecznych | 020 - Na podstawie stacji 33 |
| 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
Wszystkie czasy w UTC
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| Ostatnie rozbłyski klasy X | 2026/02/04 | X4.3 |
| Ostatnie rozbłyski klasy M | 2026/02/05 | M1.1 |
| Ostatnia burza geomagnetyczna | 2026/02/05 | Kp5+ (G1) |
| Dni bez plam słonecznych | |
|---|---|
| Ostatni dzień bez plamy słonecznej | 2022/06/08 |
| Średnia miesięczna liczba plam słonecznych | |
|---|---|
| stycznia 2026 | 112.6 -11.4 |
| lutego 2026 | 139.3 +26.7 |
| Ostatnie 30 dni | 124.9 +18 |