Het archief bekijken van donderdag 26 oktober 2023

Dagelijks bulletin over zonne- en geomagnetische activiteit van het SIDC

Datum verslag: 2023 Oct 26 1231 UTC

SIDC Prognose

Zonnevlammen

Quiet conditions (<50% probability of C-class flares)

Geomagnetisme

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

Proton Flux monitor

Quiet

10cm fluxAp
26 Oct 2023127014
27 Oct 2023129015
28 Oct 2023129010

Zonnevlekkengebieden en zonnevlammen

The solar flaring activity was at low levels, with several C-class flares recorded in the past 24 hours. There are currently only two numbered active regions on the solar disk with sunspots remaining. The largest flare was an C3.0 flare, peaking at 22:44 on Oct 25, associated with NOAA AR 3471 (beta class). NOAA AR 3468 (alpha class) did not show any significant flaring activity. The solar flaring activity is expected to be at low levels over the next 24 hours with a C-class flares possible.

Coronale massa uitstoten

No Earth directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph imagery.

Zonnewind

Over the past 24 hours, the solar wind conditions became slightly disturbed with the total interplanetary magnetic field rose to 13 nT at around 08:30 UTC on 26 Oct. The southward component of the interplanetary magnetic field ranged between -12 nT and 8 nT. The solar wind speed followed an increasing trend, rising from 310 km/s to 380 km/s. The magnetic field orientation was variable at the start of the period before switching to the predominantly positive sector (field directed away from the Sun) from 19:30 UTC on Oct 25. This might be associated with arrival of the compression region in front of the expected HSS from a positive polarity coronal hole. Solar wind parameters are expected to remain slightly elevated in the next days due to HSS arrival associated with the positive polarity coronal hole, that transited the central meridian on Oct 23.

Geomagnetisme

Geomagnetic conditions over the past 24 hours were quiet to unsettled (NOAA Kp: 1 to 3 and K-BEL: 1 to 3). Geomagnetic conditions are expected to be at quiet to unsettled levels with a chance for isolated active and minor storm periods in response to the high-speed stream arrival from a positive polarity coronal hole.

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.

Elektronenfluxen in geostationaire baan

The greater than 2 MeV electron flux remained below the 1000 pfu threshold as measured by GOES 16. It is expected to remain below this threshold over the next days. The 24 hour electron fluence was at normal levels and is expected to remain so.

Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 052, gebaseerd op 14 stations.

Zon indexen voor 25 Oct 2023

Wolfgetal Catania///
10cm zonneflux126
AK Chambon La Forêt009
AK Wingst003
Geschatte Ap002
Geschat internationaal zonnevlekkengetal031 - Gebaseerd op 16 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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Laatste alerts

04:54 UTC - Radio blackout

Kleine R1 radio blackout gedetecteerd (≥M1 - momenteel: M1.89)


04:48 UTC - Zonnevlam

Matige M1.12 zonnevlam

alert


04:24 UTC - Zonnevlam

Matige M1.13 zonnevlam

alert


04:09 UTC - Radio blackout

Kleine R1 radio blackout gedetecteerd (≥M1 - momenteel: M1.13)


01:51 UTC - Zonnevlam

Matige M1.09 zonnevlam

alert


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Ruimteweer feitjes

Laatste X-klasse uitbarsting28/03/2025X1.1
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Laatste geomagnetische storm06/04/2025Kp5 (G1)
Zonnevlekkenloze dagen
Laatste zonnevlekkenloze dag08/06/2022
Maandelijks gemiddeld zonnevlekkengetal
maart 2025134.2 -20.4
april 2025136.4 +2.2
Afgelopen 30 dagen134.7 -7.2

Deze dag in de geschiedenis*

Zonnevlammen
12024M2.41
22023C8.3
32015C6.76
42023C6.6
52015C6.17
DstG
11981-311G4
21990-108G1
31973-84G3
42001-77G3
51969-64
*sinds 1994

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