Випущено: 2018 Apr 20 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Minor storm expected (A>=30 or K=5)
Quiet
10cm flux | Ap | |
---|---|---|
20 Apr 2018 | 073 | 035 |
21 Apr 2018 | 072 | 013 |
22 Apr 2018 | 072 | 009 |
The sunspot group which appeared from the behind of the East solar limb yesterday got numbered as Catania sunspot group 78 (NOAA AR 2706). This sunspot group was source of the all (low B-class), flaring activity during last 24 hours. We expect that Catania sunspot group 78 might be the source of the B-class flares and possibly also isolated C-class flare in the following 24 hours. There were no Earth directed CMEs observed since the last report and the solar protons remain at the background level.
The in situ observations showed sudden increase of the interplanetary magnetic field magnitude (IMF), solar wind speed, density and temperature at about 23:19 UT yesterday evening. All this indicates arrival of the shock wave, however presently it is still unclear if the shock wave will be followed by the ICME or this is a shock in the solar wind related with the expected arrival of the fast flow. The shock wave was followed by gradual increase of the solar wind speed and IMF. The fast solar wind (up to 515 km/s) and longer intervals of negative values of the Bz component of the IMF (down to -19 nT), resulted in the active to storm geomagnetic conditions reported this morning (local station at Dourbes reported K=5 and NOAA reported Kp=6). The solar wind speed is presently about 480 km/s and the IMF is about 14 nT. If the solar wind speed will continue to increase and the Bz component will show longer intervals with negative values we can expect continuation of the disturbed geomagnetic conditions in the coming hours.
Today's estimated international sunspot number (ISN): 015, based on 27 stations.
Wolf number Catania | 012 |
10cm solar flux | 071 |
AK Chambon La Forêt | 011 |
AK Wingst | 002 |
Estimated Ap | 002 |
Estimated international sunspot number | 007 - Based on 39 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 |