Datum verslag: 2024 Oct 17 1231 UTC
M-class flares expected (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
10cm flux | Ap | |
---|---|---|
17 Oct 2024 | 167 | 017 |
18 Oct 2024 | 170 | 029 |
19 Oct 2024 | 175 | 018 |
Solar flaring activity was moderate over the past 24 hours, with several M-class flares identified. The largest flare was a M2.4-flare, with peak time 05:05 UTC on October 17 2024, from SIDC Sunspot Group 283 NOAA AR 3854 (beta-gamma-delta). There are currently 7 numbered active regions on the visible disk. SIDC Sunspot group 283 and 285 (NOAA AR 3854 and resp. 3856) are the most complex AR (beta-gamma- delta).The solar flaring activity is expected to be at moderate levels over the coming day with C-class flares expected and M-class flares probable and a chance of X-class flares.
A halo Coronal Mass Ejection (CME), first appeared in the SOHO/LASCO-C2 field of view at 16 OCT 23:12 UTC. An initial analysis suggests this CME is likely to have originated from the back side of the sun.
The solar wind at the Earth is slow, with speeds around 400 km/s, with a temporary slight increase to 460 km/s at 13:00 UTC on OCT 16. The interplanetary magnetic field was around 7 nT with the Bz reaching a minimum value of -7 nT. The solar wind speed is expected to become slightly enhanced on 17 OCT, due to the potential arrival of the high-speed stream (HSS) associated with the coronal hole, which crossed the central meridian on 14 OCT.
Geomagnetic conditions were quiet to unsettled (both NOAA Kp and local K Belgium 3) over the past 24 hours. Geomagnetic conditions are expected to reach active levels on OCT 17, due to a high-speed stream arrival.
The greater than 10 MeV proton flux remained below the 10 pfu threshold and is expected to remain so over the next days.
The greater than 2 MeV electron flux as measured by GOES 18 was shortly above the 1000 pfu alert threshold on OCT16 18:20 UTC, and has a small chance to exceed this level again shortly during the next 24 hours. The 24h electron fluence was at nominal levels and is expected to remain so.
Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 137, gebaseerd op 13 stations.
Wolfgetal Catania | /// |
10cm zonneflux | 168 |
AK Chambon La Forêt | 020 |
AK Wingst | 017 |
Geschatte Ap | 016 |
Geschat internationaal zonnevlekkengetal | 121 - Gebaseerd op 18 stations |
Dag | Start | Max | Einde | Locatie | Sterkte | OP | 10cm | Catania/NOAA | Soorten radio-uitbarstingen |
---|---|---|---|---|---|---|---|---|---|
16 | 0312 | 0319 | 0338 | ---- | M3.0 | 42/3852 | II/3 | ||
16 | 0338 | 0346 | 0359 | ---- | M3.7 | 42/3852 | II/3 | ||
16 | 0457 | 0515 | 0529 | S12W35 | M2.8 | 1N | 42/3852 | I/2 | |
16 | 1312 | 1327 | 1338 | S09W44 | M1.5 | 1 | 42/3852 | ||
16 | 1429 | 1442 | 1451 | S09W43 | M1.3 | 1N | 42/3852 | 38 | |
16 | 1451 | 1500 | 1504 | S05W45 | M1.3 | 1 | 42/3852 |
Aangeboden door het Solar Influences Data Analysis Center© - SIDC - Verwerkt door SpaceWeatherLive
Alle tijden in UTC
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