Випущено: 2022 Oct 22 1237 UTC
C-class flares expected, (probability >=50%)
Minor storm expected (A>=30 or K=5)
Quiet
10cm flux | Ap | |
---|---|---|
22 Oct 2022 | 109 | 023 |
23 Oct 2022 | 110 | 035 |
24 Oct 2022 | 110 | 034 |
Solar flaring activity was at low levels. The largest flare recorded was a C6.4-class flare, originating from beyond the west limb with peak time of 05:42 UTC on October 22. A new active region emerged in the south-west quadrant during the period, numbered NOAA AR3128, but did not produce any significant flaring activity. The two remaining active regions, NOAA 3127 and NOAA 3126, grew slightly. For the next 24 hours, C-class flares are expected, with a small chance for an M-class flare.
No Earth-directed Coronal Mass Ejections were observed in the last 24 hours.
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 reached the 1000 pfu alert threshold on October 21 before decreasing. It is expected to be below threshold during the next 24 hours. The 24h electron fluence was at nominal levels over the past 24 hours and is expected to remain at this level in the next 24 hours.
Over the past 24 hours, the solar wind speed ranged between 340 and 390 km/s. The total magnetic field (Bt) increased from 5 to 12 nT, while its Bz component reached -10nT. The interplanetary magnetic field phi angle switched from being in the negative sector (directed towards the Sun) to the positive sector(directed away from the Sun). Over the next 24 hours, the interplanetary magnetic field values are expected to remain enhanced. Another high-speed stream is also expected from October 23 associated with the negative polarity coronal hole, which began to cross the central meridian on October 20.
Geomagnetic conditions reached minor storm conditions 22 October 09-12 UTC (NOAA Kp 5 and local K-dourbes 4 ). In the next 24 hours the conditions are expected to be active, with moderate storm conditions possible.
Today's estimated international sunspot number (ISN): 061, based on 12 stations.
Wolf number Catania | 070 |
10cm solar flux | 109 |
AK Chambon La Forêt | 010 |
AK Wingst | 004 |
Estimated Ap | 003 |
Estimated international sunspot number | 053 - Based on 20 stations |
Day | Begin | Max | Кінець | Loc | Strength | OP | 10cm | Catania/NOAA | Radio burst types | |
---|---|---|---|---|---|---|---|---|---|---|
Немає |
Provided by the Solar Influences Data analysis Center© - SIDC - Processed by SpaceWeatherLive
Весь час у UTC
Багато людей відвідують сайт SpaceWeatherLive, щоб слідкувати за сонячною та авроральною активністю, але зі збільшенням трафіку хостинг також стає дорожчим. Будь-ласка, подумайте про пожертву, якщо вам подобається SpaceWeatherLive, щоб ми могли і надалі підтримувати цей сайт і платити за хостинг!
Останній X-спалах | 2025/03/28 | X1.1 |
Останній M-спалах | 2025/04/01 | M5.6 |
Останній геомагнітний шторм | 2025/03/27 | Kp5 (G1) |
Дні без сонячних плям | |
---|---|
Останній день без сонячних спалахів | 2022/06/08 |
Середня кількість сонячних плям протягом місяця | |
---|---|
лютого 2025 | 154.6 +17.6 |
Останні 30 днів | 128.5 -22.7 |