Het archief bekijken van maandag 30 december 2024

Dagelijks bulletin over zonne- en geomagnetische activiteit van het SIDC

Datum verslag: 2024 Dec 30 1234 UTC

SIDC Prognose

Zonnevlammen

M-class flares expected (probability >=50%)

Geomagnetisme

Quiet (A<20 and K<4)

Proton Flux monitor

Warning condition (activity levels expected to increase, but no numeric forecast given)

10cm fluxAp
30 Dec 2024255007
31 Dec 2024250019
01 Jan 2025245039

Zonnevlekkengebieden en zonnevlammen

Solar flaring activity was at high levels over the past 24 hours with 2 X-class flares being recorded and multiple M-class flares. There are a total of 11 numbered sunspot groups on the solar disk. SIDC Sunspot Group 349 (NOAA Active Region 3936) is the most complex with a Beta-Gamma-Delta magnetic configuration and produced the largest flare, an X1.5 flare (SIDC Flare 3128), peaking on December 30 at 04:14 UTC. The second X-class flare was an X1.1 flare (SIDC Flare 3130), with peak time 04:31 UTC on December 30, associated with SIDC Sunspot Group 341 (NOAA Active Region 3932). SIDC Sunspot Groups 346, 350, 351 and 352 (NOAA ARs 3933, 3938, 3939 and 3941, respectively) all produced M-class flaring activity over the last 24 hours. SIDC Sunspot Group 346 is now about to rotate over the west solar limb. The solar flaring activity is expected to be moderate over the next 24 hours, with C-class flares expected, M-class flares likely and further X-class flares possible.

Coronale massa uitstoten

The halo Coronal Mass Ejection (CME) reported yesterday, seen in SOHO/LASCO-C2 data from 06:12 UTC December 29 has been further analysed and is likely associated with the M2 flare (SIDC flare 3113) at 04:30 UTC December 29 associated with SIDC Sunspot Group 351 (NOAA AR 3939). An eruption and dimming can be seen in the south-east of the solar disk seen in SUVI 305 images around 05:00 UTC. This CME is deemed to be Earth directed with an estimated arrival time of late on December 31. A second faint partial halo CME directed to the east was also observed in SOHO/LASCO-C2 data from 18:12 UTC on December 29, associated with a on disk dimming and eruption visible in the south-east quadrant also near SIDC Sunspot Group 351 (NOAA AR 3939) in SUVI 94 and 305 imagery. Although faint and difficult to analyse this CME is also determined to be Earth directed with an estimated arrival on January 01.

Zonnewind

Over the past 24 hours the solar wind conditions reflected a slow solar wind regime. The interplanetary magnetic field ranged between 2 and 9 nT, with a minimum Bz of -7 nT. The solar wind speed ranged between 330 km/s and 400 km/s. The interplanetary magnetic field phi angle switched multiple times between the negative and positive sectors. Slow solar wind conditions are expected to continue to dominate on December 30, with an enhancement of the solar wind speed and magnetic field expected from late on December 31 due to the anticipated arrival of the CME observed on December 29.

Geomagnetisme

The geomagnetic conditions over the past 24 hours were quiet to unsettled. Quiet to unsettled geomagnetic conditions are expected for the next 24 hours, with minor to moderate geomagnetic storm conditions possible from late on December 31 due to the anticipated CME arrival.

Proton flux niveaus

The greater than 10 MeV GOES proton flux was below the 10 pfu threshold and is expected to remain so. However, due to the number of complex regions on disk and the high flaring probability a possible proton event over the next days cannot be excluded.

Elektronenfluxen in geostationaire baan

The greater than 2 MeV electron flux as measured by GOES 18 was below the 1000 pfu threshold and is expected to remain below this threshold over the next 24 hours. The 24h electron fluence was at nominal levels and is expected to remain so in the next 24 hours.

Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 226, gebaseerd op 06 stations.

Zon indexen voor 29 Dec 2024

Wolfgetal Catania///
10cm zonneflux255
AK Chambon La Forêt007
AK Wingst005
Geschatte Ap004
Geschat internationaal zonnevlekkengetal265 - Gebaseerd op 09 stations

Overzicht opvallende gebeurtenissen

DagStartMaxEindeLocatieSterkteOP10cmCatania/NOAASoorten radio-uitbarstingen
29121512241229N10W36M1.6SF69/3936
29125012561300N10W37M1.3S69/3936
29150215091522----M7.169/3936II/1
29165617081720N19E01M3.3S74/3939II/1TM/1
29174617521758S12W47M1.2SN68/3932II/2
29175818041808S06E29M1.4SF75/39403
29182718411858N13W40M3.31N--/3934
29203120392046S06W76M1.1SF67/3933
29214221532157S16E18M1.5S69/3936
29215722062213----M1.869/3936
29232023302336S16E18M1.9S74/3939III/1
30003300470058S17E19M1.7SF74/3939VI/2III/1
30025003000308S05E25M1.7SF--/3940
30040104140428N10W45X1.52N69/3936
30042904310434S19W50X1.1168/3932
30061306250640N11W47M3.5SF69/3936
30083408400844S09W55M1.4SF67/3933VI/2
30084408500856----M1.767/3933III/1
30100010111018S16E12M1.7SF67/3933

Aangeboden door het Solar Influences Data Analysis Center© - SIDC - Verwerkt door SpaceWeatherLive

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