Випущено: 2019 Oct 24 1230 UTC
Quiet conditions (<50% probability of C-class flares)
Minor storm expected (A>=30 or K=5)
Quiet
10cm flux | Ap | |
---|---|---|
24 Oct 2019 | 065 | 036 |
25 Oct 2019 | 065 | 040 |
26 Oct 2019 | 065 | 022 |
Solar X ray flux remained below B level throughout the period. There are no active regions on disk and X-ray flux is expected to remain at background levels.
No Earth-directed CME's were detected in coronagraph images.
Solar high energy proton fluxes were at background levels and are expected to remain so.
Solar wind parameters showed this morning the expected arrival of the compression region ahead of the recurrent high speed stream. Total magnetic field reached a peak over 13nT around 9UT. The Bz was mostly negative with peaks down to -11nT. The magnetic field phi angle remained in the negative sector before switching to the positive sector around 11UT. The Solar wind speed increased to over 520km/s and is still rising. The Solar wind speed is expected to further increase and remain elevated for the next 24-48 hours before starting to subside.
Until just recently, geomagnetic conditions were quiet (NOAA Kp and local K Dourbes 0-2). The latest synoptic period 9-12UT showed active geomagnetic levels (NOAA Kp and local K Dourbes 4) as expected under the Solar wind perturbations. Geomagnetic conditions are expected to be active with minor geomagnetic storms and possibly a moderate geomagnetic storm period over the next 24-48 hours, before easing to unsettled to active levels.
Today's estimated international sunspot number (ISN): 000, based on 16 stations.
Wolf number Catania | 000 |
10cm solar flux | 065 |
AK Chambon La Forêt | /// |
AK Wingst | /// |
Estimated Ap | 003 |
Estimated international sunspot number | 000 - Based on 23 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 |