Het archief bekijken van maandag 4 december 2023

Dagelijks bulletin over zonne- en geomagnetische activiteit van het SIDC

Datum verslag: 2023 Dec 04 1232 UTC

SIDC Prognose

Zonnevlammen

C-class flares expected, (probability >=50%)

Geomagnetisme

Active conditions expected (A>=20 or K=4)

Proton Flux monitor

Quiet

10cm fluxAp
04 Dec 2023141010
05 Dec 2023138019
06 Dec 2023135018

Zonnevlekkengebieden en zonnevlammen

Solar flaring activity was low but frequently during the past 24 hours. NOAA Active Region (AR) 3511 (magnetic configuration Beta, Catania sunspot group 79) produced the brightest flare, a C8 today at 01:26 UTC and has undergone through a very significant flux emergence during the last 24 hours. C-class flares are expected in the next 24 hours and if NOAA AR 3511 continues to increase, M-class flare(s) are likely to register.

Coronale massa uitstoten

A partial halo Coronal Mass Ejection (CME) can be seen in LASCO-C2/SOHO images starting from today 07:00 UTC. This is most likely a front-sided event and there is a good chance to become geo- effective. If so, it is expected to arrive at the first half of 7 Dec. A partial halo CME, also seen in LASCO-C2/SOHO images, appeared yesterday at 10:36 UTC. This is estimated to be back-sided event and as such not geo- effective.

Zonnewind

The Solar Wind (SW) conditions are affected by the arrival of the expected High Speed Stream (HSS) during the last 24 hours. The SW speed reached 580 km/s, while the total interplanetary magnetic field (Bt) increased from below 5 nT to 12 nT. The North-South magnetic component (Bz) ranged between -9 and 9 nT as a result of the HSS arrival. The interplanetary magnetic field phi angle was almost exclusively directed towards the Sun during the past 24 hours. The SW conditions are expected to remained strongly affected by the said HSS during the next 24 hours.

Geomagnetisme

Geomagnetic conditions were quiet to unsettled both globally and locally (NOAA Kp 3+ to 2 and K BEL 3 to 1) during the last 24 hours. They are expected to remain unsettled in the next 24 hours, possibly reaching active levels.

Proton flux niveaus

The greater than 10 MeV proton flux was at nominal levels over the past 24 hours and is expected to remain so for the next 24 hours.

Elektronenfluxen in geostationaire baan

The greater than 2 MeV electron flux, as measured by the GOES-16 satellite, was below the 1000 pfu alert threshold during the last 24 hours and is expected to to remain below this threshold during the next 24 hours. The 24h electron fluence was at low levels during the past 24 hours and is expected to remain at these levels for the following 24 hours.

Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 112, gebaseerd op 06 stations.

Zon indexen voor 03 Dec 2023

Wolfgetal Catania///
10cm zonneflux139
AK Chambon La Forêt015
AK Wingst012
Geschatte Ap011
Geschat internationaal zonnevlekkengetal109 - Gebaseerd op 15 stations

Overzicht opvallende gebeurtenissen

DagStartMaxEindeLocatieSterkteOP10cmCatania/NOAASoorten radio-uitbarstingen
Geen

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

Alle tijden in UTC

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