Het archief bekijken van vrijdag 21 juni 2024

Dagelijks bulletin over zonne- en geomagnetische activiteit van het SIDC

Datum verslag: 2024 Jun 21 1231 UTC

SIDC Prognose

Zonnevlammen

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

Geomagnetisme

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

Proton Flux monitor

Quiet

10cm fluxAp
21 Jun 2024204013
22 Jun 2024204021
23 Jun 2024204013

Zonnevlekkengebieden en zonnevlammen

Solar flaring activity over the last 24 hours has been at moderate levels, with multiple C-class and M-class flares. The largest flare was a M5.8 flare peaking at 23:13 UTC originated from NOAA active region 3719. There are currently six sunspot groups on the disc with NOAA active region 3719 producing the two M-class flares. The solar flaring activity is expected to be at low to moderate levels over the next 24 hours, with C-class flares expected, M-class flares possible and a small chance of X-class flares.

Coronale massa uitstoten

No Earth-directed coronal mass ejection (CME) was observed in SOHO/LASCO-C2 coronographe images over the last 24 hours.

Coronale gaten

A large north midlatitude north coronal hole with negative polarity, which has crossed the central meridian on June 18 is on geoeffective location, now in the west side of the sun.

Zonnewind

Solar wind conditions have returned to slow wind regime in the last 24 hours. The solar wind speed decreased from around 501 km/s to 388 km/s. The interplanetary magnetic field remained below 6 nT and the Bz component varied between -3 nT and 5 nT. The solar wind conditions are expected to remain in a slow solar wind regime. Then the high-speed stream from the large north midlatitude north coronal hole with negative polarity is expected to reach Earth in the next period.

Geomagnetisme

Geomagnetic conditions were quiet (NOAA Kp 0-2, K BEL 1-2). Later, active conditions to minor storm may be observed later in the next period, in response of the high-speed stream from the large north midlatitude north coronal hole.

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 and decrease over the next 24 hours.

Elektronenfluxen in geostationaire baan

The greater than 2 MeV electron flux was below the threshold level in the last 24 hours and is expected to remain so over the next 24 hours. The 24h 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: 148, gebaseerd op 12 stations.

Zon indexen voor 20 Jun 2024

Wolfgetal Catania///
10cm zonneflux203
AK Chambon La Forêt013
AK Wingst009
Geschatte Ap007
Geschat internationaal zonnevlekkengetal163 - Gebaseerd op 22 stations

Overzicht opvallende gebeurtenissen

DagStartMaxEindeLocatieSterkteOP10cmCatania/NOAASoorten radio-uitbarstingen
20150915181522----M1.1--/3719
20230023162320S14E57M5.71B--/3719

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

Alle tijden in UTC

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Laatste alerts

16:00 UTC - Zonnevlam

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Ruimteweer feitjes

Laatste X-klasse uitbarsting28/03/2025X1.1
Laatste M-klasse uitbarsting13/04/2025M1.2
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
22025M2.2
32025M1.3
42025M1.2
52025M1.1
DstG
11981-311G4
21990-108G1
31973-84G3
42001-77G3
51969-64
*sinds 1994

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