Випущено: 2020 May 07 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
07 May 2020 | 070 | 004 |
08 May 2020 | 070 | 004 |
09 May 2020 | 070 | 004 |
The solar activity was quiet over the past 24 hours. No sunspot is visible on the solar disc facing Earth. The X-ray flux is below B-class level and the solar activity is expected to remain at low levels.
No Earth directed Coronal Mass Ejections (CMEs) were observed in the available coronagraphic imagery 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 stay at nominal levels for the next 24 hours. The greater than 2 MeV electron flux was between nominal and moderate levels over the past 24 hours and is expected to remain at nominal to moderate levels over the next 24 hours.
The solar wind parameters recorded near Earth (DSCOVR) show nominal values. The solar wind speed was slow and oscillated between 289 km/s and 345 km/s. The total interplanetary magnetic field was below 6 nT. The Bz magnetic field components fluctuated between -4.6 nT and +4.7 nT. The slow solar wind regime is expected to remain for the next days. Later, in about 2-3 days from now, slight enhancements of the solar wind conditions may occur in response to the influence of the solar wind associated with the elongated extension of the southern polar coronal hole (negative polarity) that was facing Earth on May 6.
Geomagnetic conditions were quiet, and quiet conditions are expected for the next following days.
Today's estimated international sunspot number (ISN): 000, based on 28 stations.
Wolf number Catania | /// |
10cm solar flux | 070 |
AK Chambon La Forêt | 005 |
AK Wingst | 006 |
Estimated Ap | 005 |
Estimated international sunspot number | 000 - Based on 37 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 |