Випущено: 2021 Mar 28 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
28 Mar 2021 | 080 | 018 |
29 Mar 2021 | 080 | 017 |
30 Mar 2021 | 078 | 007 |
Solar activity was at very low levels in the past 24 hours. NOAA AR 2812 is the only active region visible, it produced only B-class flares. Solar activity is expected to remain at low levels.
No Earth directed CMEs were observed in the past 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 was below the 1000 pfu threshold in the past 24 hours and is expected to remain so during the next 24 hours. The 24h electron fluence is at normal levels in the last 24 hours and is expected to stay at normal levels for the next 24 hours.
The solar wind speed increased from 340 to 440 km/s in the last 24 hours, marking a very mild start of the expected high speed stream. The interplanetary magnetic field magnitude varied between 2 nT and 7 nT, while Bz varied between -7 nT and 6 nT in the last 24 hours. The interplanetary magnetic field phi angle had a mostly negative polarity (towards the Sun). A period between 17:00 UT and 23:00 UT shows some signatures of an ICME, including a low temperature, this could be a late arrival of the CME from 22 March (it caused active geomagnetic conditions). The solar wind speed could increase more in the next 24 hours.
Geomagnetic conditions were quiet to unsettled (Kp and KDourbes: 1-4), similar situation is expected for the next 24 hours.
Today's estimated international sunspot number (ISN): 010, based on 15 stations.
Wolf number Catania | /// |
10cm solar flux | 080 |
AK Chambon La Forêt | 019 |
AK Wingst | 007 |
Estimated Ap | 008 |
Estimated international sunspot number | 011 - 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 | M2.5 |
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 |
квітня 2025 | 147 -7.6 |
Останні 30 днів | 128.8 -21.8 |