Випущено: 2020 Nov 29 1232 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Quiet
10cm flux | Ap | |
---|---|---|
29 Nov 2020 | 111 | 004 |
30 Nov 2020 | 113 | 005 |
01 Dec 2020 | 113 | 003 |
Solar activity was at low levels in the past 24 hours. NOAA Active Region (AR) 2786 (Beta-Gamma) has been most active, producing multiple low- level C-class flares, including a C3.1 flare that peaked at 23:18 UT Nov 28. There are four further numbered active regions on the solar disk. NOAA AR 2783 (Alpha), which is now close to rotating over the west solar limb, and NOAA AR 2787 (Alpha) remained quiet. Further spot development and flux emergence to the west of NOAA 2785 at S27W05 has been designated as a separate active region, numbered NOAA AR2788 (Alpha). Another simple (Alpha) unnumbered region has also emerged at S28W55. The solar activity is expected to remain at low levels with a high chance for C-class flares, particularly from NOAA AR 2786. An isolated M-class flare also remains possible.
No Earth directed CMEs have been detected in the available coronagraphic 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 2 MeV electron flux exceeded the 1000 pfu alert threshold between 12:40 and 20:50 UT Nov 28. During the next 24 hours, the electron flux is expected to exceed the 1000 pfu level again. The 24h electron fluence was at moderate levels and is expected to be at normal to moderate levels over the next 24 hours.
Over the past 24 hours, the solar wind speed decreased from around 440 to 350 km/s (DSCOVR). The total magnetic field strength ranged between 2 and 8 nT. Bz had a minimum value of -6 nT with an extended period of negative Bz from 04:30 UT Nov 29. The interplanetary magnetic field was predominantly directed towards the Sun (phi angle in the negative sector). Over the next 24 hours, the solar wind parameters are expected to be at nominal levels.
Geomagnetic conditions were at quiet to unsettled levels over the past 24 hours (NOAA Kp and local k Dourbes recorded values of 1-3 and 0-3, respectively). Geomagnetic conditions are expected to be at quiet levels for the next 24 hours with some unsettled conditions possible in response to prolonged periods of negative Bz.
Today's estimated international sunspot number (ISN): 084, based on 13 stations.
Wolf number Catania | /// |
10cm solar flux | 110 |
AK Chambon La Forêt | 011 |
AK Wingst | 012 |
Estimated Ap | 011 |
Estimated international sunspot number | 072 - 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 | 147 -7.6 |
Останні 30 днів | 128.8 -21.8 |