Het archief bekijken van zaterdag 14 december 2024

Dagelijks bulletin over zonne- en geomagnetische activiteit van het SIDC

Datum verslag: 2024 Dec 14 1231 UTC

SIDC Prognose

Zonnevlammen

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

Geomagnetisme

Quiet (A<20 and K<4)

Proton Flux monitor

Warning condition (activity levels expected to increase, but no numeric forecast given)

10cm fluxAp
14 Dec 2024163008
15 Dec 2024161010
16 Dec 2024160007

Zonnevlekkengebieden en zonnevlammen

Solar flaring activity over the last 24 hours has been at moderate levels, with two M-class flares and several C-class flares. The strongest flare was a M1.0 flare (SIDC Flare 2949) peaking at 14:24 UTC on December 13, produced by SIDC Sunspot Group 318 (NOAA Active Region 3922, magnetic type beta). There are currently four numbered active regions on the solar disk. The most complex ones are SIDC Sunspot Group 288 (NOAA Active Region 3917, magnetic type beta-gamma-delta) and SIDC Sunspot Group 332 (NOAA Active Region 3920, magnetic type beta- delta). A new, currently unnumbered active region has rotated on disk in the northeast quadrant. SIDC Sunspot Group 288 (NOAA Active Region 3917) is currently rotating behind the west limb. SIDC Sunspot Group 334 (NOAA Active Region 3921) and SIDC Sunspot Group 336 (NOAA Active Region 3923) have decayed into plage. The solar flaring activity is expected to be at moderate levels over the next 24 hours, with M-class flares expected and a chance for X-class flares.

Coronale massa uitstoten

A coronal mass ejection (CME) was observed in LASCO/C2 coronagraph imagery around 05:36 UTC on December 14, lifting off the southwest quadrant. It is most likely associated with a filament eruption and flaring activity near SIDC Sunspot Group 288 (NOAA Active Region 3917) around 05:10 UTC on December 14. The CME is propagating to the southwest with an estimated speed of 800 km/s. Current analysis suggests a small chance that a mild glancing blow may arrive at Earth in the UTC evening on December 17. A large filament eruption was observed in GOES/SUVI 304 data around 01:45 UTC on December 14 in the southeast quadrant, near SIDC Sunspot Group 318 (NOAA Active Region 3922). A prominence eruption was observed in GOES/SUVI 304 data around 08:40 UTC at the east limb. No associated CMEs have been observed in the available coronagraph imagery. No other Earth-directed CMEs were observed in the available coronagraph imagery.

Zonnewind

Over the past 24 hours, the solar wind parameters (ACE and DSCOVR) reflected slow solar wind conditions. Speed values were between 310 and 350 km/s. The interplanetary magnetic field values were between 5 nT and 9 nT. The Bz component was mostly negative, with values varying between -6 nT and 4 nT. The interplanetary magnetic field angle was predominantly in the positive sector. Mostly slow solar wind conditions are expected over the next 24 hours, with a small chance for enhancements due to a possible high-speed stream arrival from the northern, positive polarity coronal hole (SIDC Coronal Hole 78).

Geomagnetisme

Geomagnetic conditions globally and locally were at quiet levels (NOAA Kp 2 and K BEL 2) in the last 24 hours. Quiet conditions are expected globally and locally over the next 24 hours, with a small chance for unsettled to active intervals due to the possible high-speed stream arrival from the northern, positive polarity coronal hole (SIDC Coronal Hole 78).

Proton flux niveaus

The greater than 10 MeV proton flux was below the threshold level over the past 24 hours. It is expected to remain below the threshold level over the next 24 hours, pending no further eruptive activity.

Elektronenfluxen in geostationaire baan

The greater than 2 MeV electron flux measured by GOES 16 and GOES 18 was enhanced but remained below the threshold level in the last 24 hours. It is expected to remain so over the next 24 hours. The 24-hour electron fluence is presently at normal levels and is expected to remain so over the next 24 hours.

Het geschatte internationale zonnevlekkengetal (ISN) van vandaag: 094, gebaseerd op 04 stations.

Zon indexen voor 13 Dec 2024

Wolfgetal Catania///
10cm zonneflux164
AK Chambon La Forêt008
AK Wingst003
Geschatte Ap003
Geschat internationaal zonnevlekkengetal124 - Gebaseerd op 08 stations

Overzicht opvallende gebeurtenissen

DagStartMaxEindeLocatieSterkteOP10cmCatania/NOAASoorten radio-uitbarstingen
13111311241130S08W49M2.0SF33/3917
13141514241431----M1.047/3922V/2III/2
13171417211727----M0.933/3917

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

Geen noemenswaardig ruimteweer gebeurd in de afgelopen 48 uur...
Ontvang directe meldingen!

Ruimteweer feitjes

Laatste X-klasse uitbarsting28/03/2025X1.1
Laatste M-klasse uitbarsting22/04/2025M1.3
Laatste geomagnetische storm21/04/2025Kp5+ (G1)
Zonnevlekkenloze dagen
Laatste zonnevlekkenloze dag08/06/2022
Maandelijks gemiddeld zonnevlekkengetal
maart 2025134.2 -20.4
april 2025124.6 -9.6
Afgelopen 30 dagen122.9 -6.2

Deze dag in de geschiedenis*

Zonnevlammen
12001X1.13
22003X1
32003M3.71
42003M3.05
52003M3.02
DstG
11989-132G3
21984-93G4
31981-85G3
41979-80
51960-72
*sinds 1994

Sociale netwerken