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Dagelijks bulletin over zonne- en geomagnetische activiteit van het SIDC

Datum verslag: 2024 Feb 23 1231 UTC

SIDC Prognose

Zonnevlammen

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

Geomagnetisme

Quiet (A<20 and K<4)

Proton Flux monitor

Quiet

10cm fluxAp
23 Feb 2024176013
24 Feb 2024180007
25 Feb 2024184010

Zonnevlekkengebieden en zonnevlammen

Solar flaring activity over the past 24 hours was at high levels, with one X-class flares and one M-class flare. The largest flare was a X6.3-flare, with peak time 22:34 UTC on February 22 and the second largest flare was a M4.8-flare, with peak time 20:46 UTC on February 22. Both flares were associated with NOAA AR 3590 (beta-gamma- delta). The third largest flare a C9.4-flare, with peak time 16:29 UTC on February 22 was produced by a yet unnumbered active region behind the east- limb. There are currently 2 numbered active regions on the visible disk. NOAA AR 3590 (beta-gamma-delta) is the largest, most magnetically complex region and has produced most of the flaring activity in the last 24 hours. NOAA AR 3586 (alfa) has been stable and inactive. The solar flaring activity is likely to be at moderate levels over the coming days with C-class flares expected and M-class flares probable and a chance for an X-class flare.

Coronale massa uitstoten

No Earth directed Coronal Mass Ejections (CME)s have been observed in the last 24 hours.

Coronale gaten

Two negative polarity coronal holes are crossing the central meridian. One in the northern half of the Sun at high latitude and the other in the Southern half at low latitude. A high-speed stream from the southern coronal hole is expected to impact the Earth early on the 25th of November.

Zonnewind

Slow solar wind conditions were recorded over the past 24 hours. The solar wind speed as measured by ACE fluctuated between 304 km/s to 368 km/s. The interplanetary magnetic field fluctuated between 1 nT and 7 nT, with the Bz reaching a minimum value of -5 nT. The phi-angle was in the positive sector (directed away the Sun) with periods on the negative sector. In the next 24-hours slow solar wind conditions are expected.

Geomagnetisme

Geomagnetic conditions were globally and locally quiet (Kp 3 and K Bel 3) with some unsettled periods over the past 24 hours.

Proton flux niveaus

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. Some enhancements are possible in the case of an eruptive activity from NOAA AR 3590.

Elektronenfluxen in geostationaire baan

The greater than 2 MeV GOES 16 electron flux was below the 1000 pfu threshold and is expected to remain so in the upcoming days. The 24h electron fluence was at nominal level and is expected to remain so in the next days.

Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 102, gebaseerd op 08 stations.

Zon indexen voor 22 Feb 2024

Wolfgetal Catania073
10cm zonneflux173
AK Chambon La Forêt007
AK Wingst005
Geschatte Ap004
Geschat internationaal zonnevlekkengetal054 - Gebaseerd op 12 stations

Overzicht opvallende gebeurtenissen

DagStartMaxEindeLocatieSterkteOP10cmCatania/NOAASoorten radio-uitbarstingen
22202920462103N18E29M4.82B85/3590
22220822342243----X6.385/3590III/1

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

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Ruimteweer feitjes

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Zonnevlekkenloze dagen
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Maandelijks gemiddeld zonnevlekkengetal
maart 2025134.2 -20.4
april 2025139.5 +5.3
Afgelopen 30 dagen135.8 -6.1

Deze dag in de geschiedenis*

Zonnevlammen
12024M2.41
22023C8.3
32015C6.76
42023C6.6
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DstG
11981-311G4
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*sinds 1994

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