Het archief bekijken van zondag 31 december 2023

Dagelijks bulletin over zonne- en geomagnetische activiteit van het SIDC

Datum verslag: 2023 Dec 31 1304 UTC

SIDC Prognose

Zonnevlammen

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

Geomagnetisme

Minor storm expected (A>=30 or K=5)

Proton Flux monitor

Quiet

10cm fluxAp
31 Dec 2023138003
01 Jan 2024140030
02 Jan 2024140015

Zonnevlekkengebieden en zonnevlammen

The solar flaring activity remained at low levels with two impulsive high C-class flares produced from behind the north-east limb, possibly by returning region NOAA 3527. The strongest activity was a C9.7 flare with peak time 08:17 UTC on Dec 31st. This region is now rotating onto disc and, together with NOAA AR 3530 from behind the west limb, was responsible for most of the flaring activity over the past 24 hours. There are only three numbered active regions on the visible disc with NOAA AR 3534 (beta-gamma) being the most complex one with largest number of sunspots. It has undergone slight development, but nevertheless remained quiet and inactive. The solar flaring activity is expected to be at low levels over the coming days with probable C-class flares and some chances for isolated M-class flaring.

Coronale massa uitstoten

A partial halo coronal mass ejection (CME) was detected in the LASCO/C2 imagery after 07:00 UTC on Dec 30th. The CME is associated with a filament eruption and related long-duration C2.6 flaring from NOAA AR 3534 (beta). Coronal dimming is observed in the south-east quadrant after 08:00 UTC on Dec 30th. While the bulk of the eruption is off the Sun-Earth line, a minor glancing blow could impact Earth during the UTC night of Jan 2nd or UTC morning of Jan 3rd. The large filament in the north-west quadrant has erupted once again and appears related to a CME with coronal dimming observed after 09:00 UTC on Dec 31st. We are awaiting for coronagraph data to analyse the event. No other Earth-directed CMEs have been detected in the available coronagraph imagery over the past 24 hours.

Coronale gaten

The long negative polarity coronal hole which resided on the central meridian in the past few days starts to slowly move westward. The high speed stream related to this coronal hole could arrive to Earth late on Dec 31st or early Jan 1st and is expected to last for several days.

Zonnewind

Over the past 24 hours the solar wind parameters (ACE and DSCOVR) registered nominal slow solar wind conditions. The solar wind velocity varied in the range of 273 to 480 km/s. The interplanetary magnetic field had a maximum value of 8 nT with a minimum Bz of -4 nT. The B field was solely in the negative sector (directed towards the Sun). The solar wind conditions in the next 24 hours are expected to registered disturbances due to expected high speed stream arrival later tonight or on Jan 1st. Disturbed conditions are expected to continue throughout Jan 2nd with a possible further enhancement on Jan 3rd subject to a minor glancing blow arrival from the partial halo CME on Dec 30th.

Geomagnetisme

The geomagnetic conditions over the past 24 hours were quiet. Mostly quiet geomagnetic conditions are expected for Dec 31st. Quiet to active conditions with likely minor storm levels and possible isolated moderate storms are anticipated for Jan 1st. Quiet to active conditions with possible minor storms are expected for Jan 2nd and Jan 3rd.

Proton flux niveaus

Over the past 24 hours the greater than 10 MeV GOES proton flux was at background levels and is expected to continue so over the next days.

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: 050, gebaseerd op 09 stations.

Zon indexen voor 30 Dec 2023

Wolfgetal Catania///
10cm zonneflux140
AK Chambon La Forêt006
AK Wingst004
Geschatte Ap003
Geschat internationaal zonnevlekkengetal068 - 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

<< Keer terug naar de dagelijkse overview pagina

Op basis van de huidige parameters is er nu geen kans op poollicht in België en Nederland

Laatste nieuws

Steun Poollicht.be!

Om ook bereikbaar te blijven bij grote poollichtkansen hebben we een zware server nodig die alle bezoekers aankan. Doneer en steun dit project zodat we online blijven en je geen enkele poollichtkans mist!

Donneer SpaceWeatherLive Pro
Steun SpaceWeatherLive met onze merchandise
Check nu onze merchandise

Laatste alerts

vrijdag 9 mei 2025
20:00 UTC - Geomagnetische activiteit

Actieve geomagnetische condities (Kp4) Drempel bereikt: 19:56 UTC

alert


16:48 UTC - Hemisferisch vermogen

Het OVATION-model voorspelt dat het hemisferisch vermogen 50GW zal bereiken om 17:42 UTC


donderdag 8 mei 2025
22:45 UTC - Geomagnetische activiteit

Actieve geomagnetische condities (Kp4) Drempel bereikt: 22:34 UTC

alert


Ontvang directe meldingen!

Ruimteweer feitjes

Laatste X-klasse uitbarsting28/03/2025X1.1
Laatste M-klasse uitbarsting30/04/2025M2.03
Laatste geomagnetische storm03/05/2025Kp5 (G1)
Zonnevlekkenloze dagen
Laatste zonnevlekkenloze dag08/06/2022
Maandelijks gemiddeld zonnevlekkengetal
april 2025140.6 +6.4
mei 202578.8 -61.8
Afgelopen 30 dagen104.1 -33.5

Deze dag in de geschiedenis*

Zonnevlammen
12024X3.98
22022X1.51
32012M8.25
42024M5.97
52013M5.67
DstG
12024-351G4
21992-288G4
31981-99G3
41993-91G2
52003-84G3
*sinds 1994

Sociale netwerken