Випущено: 2023 Oct 28 1231 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
28 Oct 2023 | 126 | 017 |
29 Oct 2023 | 128 | 022 |
30 Oct 2023 | 128 | 027 |
The solar flaring activity was at low levels, with several C-class flares recorded in the past 24 hours. The largest flare was a C1.7 flare, peaking at 06:27 on Oct 28. The flare was associated with NOAA AR 3473 (beta class), which produced most of the flaring activity over the period. Other regions on the disc have simple configuration of their photospheric magnetic field (alpha and beta) and did not show any significant flaring activity. The solar flaring activity is expected to be at low level over the next 24 hours with C-class flares likely.
No Earth directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph imagery.
Over the past 24 hours, the solar wind conditions became slightly disturbed with the total interplanetary magnetic field rose to 13 nT at around 06:50 UTC on Oct 28. The southward component of the interplanetary magnetic field ranged between -8 nT and 6 nT. The solar wind speed followed an increasing trend, rising from 345 km/s to 480 km/s. The magnetic field orientation was predominantly in the positive sector (field directed away from the Sun). Solar wind parameters are expected to remain slightly elevated during the next days, with a further enhancement possible on Oct 29 - 30 due to the arrival of a high-speed stream from a positive polarity coronal holes.
The geomagnetic conditions over the past 24 hours were mostly quiet to unsettled (NOAA-Kp=1-3) with a single active period registered globally (NOAA-Kp=4) during the interval 09-12 UTC on Oct 28. Locally only quiet to unsettled (K-Bel=1-3) conditions were observed over Belgium. Unsettled conditions with possible active and minor storm intervals are expected on Oct 28 and the start of Oct 29. Geomagnetic conditions are expected to be at unsettled to active levels, with a chance for isolated minor to moderate storm period from late on Oct 29 with expected high speed stream arrival from a positive polarity coronal holes.
Over the past 24 hours the greater than 10 MeV GOES proton flux was at nominal levels and is expected to remain so over the next days.
The greater than 2 MeV electron flux remained below the 1000 pfu threshold as measured by GOES 16. It is expected to remain below this threshold over the next days. The 24 hour electron fluence was at normal levels and is expected to remain so.
Today's estimated international sunspot number (ISN): 051, based on 11 stations.
Wolf number Catania | 103 |
10cm solar flux | 128 |
AK Chambon La Forêt | 014 |
AK Wingst | 011 |
Estimated Ap | 037 |
Estimated international sunspot number | 062 - Based on 17 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
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