Випущено: 2021 Apr 17 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Minor storm expected (A>=30 or K=5)
Quiet
10cm flux | Ap | |
---|---|---|
17 Apr 2021 | 077 | 032 |
18 Apr 2021 | 078 | 018 |
19 Apr 2021 | 077 | 011 |
Solar activity remained at very low levels over the last 24 hours. Three numbered sunspot groups are visible on the solar disk, namely Catania 86 (NOAA 2814), NOAA 2815 and NOAA 2016. All of them are classified as magnetic type Beta and have shown low levels of activity with B-class flaring. The flaring activity within the next 24 hours is expected to remain low with 30% chance for C-class flares.
No Earth-directed coronal mass ejections (CMEs) were detected in the available coronagraph imagery.
The greater than 10 MeV proton flux was at nominal levels in the past 24 hours and is expected to remain so in the next 24 hours. The greater than 2MeV electron flux remained under the 1000 pfu threshold and is expected to show some enhancement. The 24h electron fluence was at nominal levels and is expected to be at nominal to moderate levels in the next 24 hours.
Over the past 24 hours the solar wind parameters (ACE and DSCOVR) were elevated with the arrival of the high speed stream (HSS) from the high- latitude extension of the negative-polarity polar coronal hole. The total magnetic field registered a magnitude of 13 nT with a minimum Bz of -11 nT. The solar wind speed varied between 400 km/s and 610 km/s. The solar wind speed is expected to remain elevated throughout April 17th.
Due to the HSS and prolonged intervals with negative Bz multiple periods with minor geomagnetic storms were registered over the past 24 hours. Unsettled to active geomagnetic conditions with more periods of minor geomagnetic storms can be expected for the next 24 hours.
Today's estimated international sunspot number (ISN): 019, based on 21 stations.
Wolf number Catania | /// |
10cm solar flux | 077 |
AK Chambon La Forêt | 038 |
AK Wingst | 020 |
Estimated Ap | 020 |
Estimated international sunspot number | 037 - Based on 26 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 |