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Coronal mass ejection impact, New website feature!

venerdì, d.C. maggio PM 17:03 UTC

Coronal mass ejection impact, New website feature!

A coronal mass ejection impact was detected at DSCOVR around 12:40 UTC today. The north-south direction of the interplanetary magnetic field (Bz) flipped southward to about -12nT to -12nT. A minor G1 geomagnetic storm watch is in effect for the remainder of the day.

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More X-flares!

mercoledì, d.C. maggio PM 18:40 UTC

More X-flares!

Sunspot region 3664 continues producing major solar flares even now that it rotated behind the west limb. An X3.4 solar flare that peaked at 08:37 UTC was highly eruptive and an impressive coronal mass ejection could be seen on LASCO coronagraph imagery from SOHO. The coronal mass ejection is however, as you might have guessed already, not aimed at our planet.

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X8.7 solar flare

martedì, d.C. maggio PM 19:42 UTC

X8.7 solar flare

What a way to sign off! Sunspot region 3664 (R3-strong) is now on the west limb and waves goodbye by producing the largest solar flare of Solar Cycle 25 which peaked at X8.7! Wow! There isn't any coronagraph imagery available from SOHO yet, but we do know the solar flare was eruptive but based on coronagraph imagery from STEREO A, the resulting coronal mass ejection is likely not aimed at Earth.

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M6.6 solar flare with earth-directed CME

lunedì, d.C. maggio PM 18:46 UTC

M6.6 solar flare with earth-directed CME

Sunspot region 3664 is now close to the west limb and quieted down a bit compared to last week. Nonetheless it was the source of an eruptive long duration M6.6 solar flare (R2-moderate) that peaked at 9:44 UTC.

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Small CME impact, Record visitor amount

domenica, d.C. maggio AM 10:12 UTC

Small CME impact, Record visitor amount

Geomagnetic conditions have subsided considerably since the intense storm conditions during 10 and 11 May. Storm conditions that several times reached the Extreme G5 geomagnetic storm threshold and rivaled the 2003 Halloween Solar Storms.

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Strongest geomagnetic storm since 2003, X5.8 solar flare

sabato, d.C. maggio PM 13:08 UTC

Strongest geomagnetic storm since 2003, X5.8 solar flare

The geomagnetic storm that commenced yesterday will go down in the record books as the strongest geomagnetic storm since the Halloween Solar Storms of 2003. The May 2024 storms thus far peaked at a Dst of -412 nT.

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Extreme G5 geomagnetic storm

sabato, d.C. maggio AM 00:14 UTC

Extreme G5 geomagnetic storm

For the first time since the Halloween Solar Storms of 2003 we have now officially reached the Extreme G5 geomagnetic storm threshold at 22:54 UTC.

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Severe G4 geomagnetic storm

venerdì, d.C. maggio PM 22:12 UTC

Severe G4 geomagnetic storm

Intense geomagnetic storm conditions continue with yet another period where we reached the severe G4 geomagnetic storm level which equals a Kp of 8. Aurora displays have been reported from all over Europe. Even locations as far south as Austria and Switzerland are seeing some amazing aurora as you can see on this image overlooking the Swiss alps.

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Coronal mass ejection impact, Severe G4 geomagnetic storm possible!

venerdì, d.C. maggio PM 17:04 UTC

Coronal mass ejection impact, Severe G4 geomagnetic storm possible!

Impact! The first of a total of up to six coronal mass ejections has now arrived at the DSCOVR satellite and will arrive at Earth within the next 30 minutes.

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CME impact imminent, Two more earth-directed CMEs

venerdì, d.C. maggio PM 15:46 UTC

CME impact imminent, Two more earth-directed CMEs

A quick update on the current solar activity and the expected geomagnetic conditions in the coming days.

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Notizie sul meteo spaziale

Ultimo brillamento X2024/11/06X2.39
Ultimo brillamento M2024/11/13M1.7
Ultima tempesta geomagnetica2024/11/10Kp5+ (G1)
Giorni senza macchie
Ultimo giorno senza macchie2022/06/08
Media mensile Numero di Macchie Solari
ottobre 2024166.4 +25
novembre 2024166 -0.4
Last 30 days163.2 +18.4

Questo giorno nella storia*

Brillamenti solari
11999X1.15
21999M8.06
32005M5.58
41999M4.11
52005M3.72
DstG
11960-167G3
21998-109G2
32012-108G2
41989-105
51979-90G1
*dal 1994

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