Het archief bekijken van dinsdag 28 november 2023

Dagelijks bulletin over zonne- en geomagnetische activiteit van het SIDC

Datum verslag: 2023 Nov 28 1230 UTC

SIDC Prognose

Zonnevlammen

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

Geomagnetisme

Quiet (A<20 and K<4)

Proton Flux monitor

Quiet

10cm fluxAp
28 Nov 2023177006
29 Nov 2023173005
30 Nov 2023165004

Zonnevlekkengebieden en zonnevlammen

Solar flaring activity was low during the past 24 hours. The brightest flare was a C6 from NOAA Active Region (AR) 3500 (magnetic configuration Beta-Gamma, Catania group 65) that peaked yesterday, 18:53 UTC. More C-class flaring activity is expected with a small chance of an isolated M-class flare in the next 24 hours.

Coronale massa uitstoten

A partial halo Corona Mass Ejection (CME) can be seen in LASCO-C2/SOHO images starting from yesterday 18:48 UTC. It is expected to be geo-effective and arrive on 1 Dec. Another CME associated with a filament eruption can be seen in LASCO-C2/SOHO images starting from 23:48 UTC, yesterday. Based on the location and extent of the filament, it is expected to arrive at Earth's environment early on Dec 1. These two events, together with the possible arrival of a CME reported yesterday, are likely to merge together and cause a strong single effect in the first half of 1 Dec.

Zonnewind

The Solar Wind (SW) conditions remained stable during the last 24 hours. The SW speed varied from 420 to 510 km/s, while the total interplanetary magnetic field (Bt) was between 3 and 6 nT. The North-South magnetic component (Bz) ranged between -5 and 4 nT, while the interplanetary magnetic field phi angle was mostly directed away from the Sun in the past 24 hours. The SW conditions are expected to remain in the slow SW regime for the next 24 hours.

Geomagnetisme

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

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 at nominal levels during the last 24 hours and is expected to remain below the 1000 pfu threshold during the next 24 hours. The 24h electron fluence was at very 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: 148, gebaseerd op 21 stations.

Zon indexen voor 27 Nov 2023

Wolfgetal Catania215
10cm zonneflux187
AK Chambon La Forêt016
AK Wingst008
Geschatte Ap008
Geschat internationaal zonnevlekkengetal166 - Gebaseerd op 11 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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