Випущено: 2020 Jun 27 1256 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
27 Jun 2020 | 068 | 008 |
28 Jun 2020 | 068 | 003 |
29 Jun 2020 | 068 | 002 |
Solar flaring activity was at very low levels. A small negative to positive sunspot appeared and decayed on the Northern West hemisphere. No significant flares have been recorded. Solar activity is expected to remain at very low levels.
No Earth directed Coronal Mass Ejections (CMEs) were observed in the available coronagraphic imagery.
The greater than 10 MeV proton flux and the greater than 2 MeV electron flux were at background levels the past 24 hours. They are expected to remain so in the next 24 hours.
The solar wind speed near Earth oscillated between 290 and 360 km/s (DSCOVR+ACE) while the density also increased. We seem to be seeing the influence of the CH crossing central meridian on June 23rd. The polarity of the Interplanetary Magnetic Field (IMF) was predominantly oriented towards the Sun (phi angle in the negative sector), switching to positive when some transient positive features crossed the disk. Bz fluctuated between -8 and +9 nT. The magnitude of the magnetic field varied between 1 and 11 nT. A filament eruption was observed at SDO/AIA close to the southern Pole and central meridian on June 26th 21:18UT. For the next 24 hours the solar wind speed is expected to continue on this trend.
Quiet to unsettled geomagnetic conditions were registered for the past 24 hours (K Dourbes and NOAA Kp recorded values 1-3). Quiet to unsettled (K Dourbes = 3) geomagnetic conditions are expected for the next 24 hours.
Today's estimated international sunspot number (ISN): 003, based on 20 stations.
Wolf number Catania | 011 |
10cm solar flux | 068 |
AK Chambon La Forêt | 015 |
AK Wingst | 009 |
Estimated Ap | 008 |
Estimated international sunspot number | 006 - Based on 35 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 | 152.5 -2.1 |
Останні 30 днів | 130.7 -17.9 |