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Let's compare! Halloween 2003 VS May 2024 Solar Storms!

Today we have a really special news item for you! We have a guest post made by Christian Harris from Space Weather Trackers. Christian is a friend of the website an has made very well received guest posts before. He has some serious big brain knowledge about everything space weather related. I am sure many of you have heard of him before. He is here to shed some light on the Extreme G5 geomagnetic storm of last weekend and the famous Halloween 2003 solar storms. Please read his article below and gain some fascinating insights on two of the strongest solar storms in modern times. It is well worth the read! If you are interested in Christian's work be sure to follow him on Facebook and follow his Space Weather Trackers Facebook page. Christian, the stage is yours:

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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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G1 - Minor geomagnetic storm

Observed Kp: 5
Threshold reached: 23:35 UTC

Current data suggests there is a high possibility for aurora to appear at the following high latitude regions in the near future

Iqaluit, NU
Nuuk
Tórshavn
Oulu, Rovaniemi, Sodankylä
Reykjavik
Tromsø
Kiruna, Luleå

Current data suggests there is a moderate possibility for aurora to appear at the following high latitude regions in the near future

Trondheim
Sundsvall, Umeå

Current data suggests there is a slight possibility for aurora to appear at the following high latitude regions in the near future

Kuopio
Bergen

Current data suggests there is a slight possibility for aurora to appear at the following middle latitude regions in the near future

Thunder Bay, ON
Tampere, Turku
Petrozavodsk
The solar wind speed is currently moderately high (506.6 km/sec.)
The strength of the interplanetary magnetic field is high (21.12nT), the direction is slightly South (-7.89nT).

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00:18 UTC - Hemispheric Power Index

The OVATION model predicts the Hemispheric Power Index to reach 101GW at 01:06 UTC


Friday, 21 March 2025
23:45 UTC - Geomagnetic activity

Minor G1 geomagnetic storm (Kp5) Threshold Reached: 23:30 UTC

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23:12 UTC - Hemispheric Power Index

The OVATION model predicts the Hemispheric Power Index to reach 77GW at 00:01 UTC


19:39 UTC - Hemispheric Power Index

The OVATION model predicts the Hemispheric Power Index to reach 53GW at 20:34 UTC


19:00 UTC - Geomagnetic activity

Minor G1 geomagnetic storm (Kp5) Threshold Reached: 18:55 UTC

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Last X-flare2025/02/23X2.0
Last M-flare2025/03/21M1.2
Last geomagnetic storm2025/03/14Kp6- (G2)
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Last spotless day2022/06/08
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February 2025154.6 +17.6
March 2025138.4 -16.2
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Solar flares
12000X1.56
22024M4.3
32000M2.86
42002M2.37
52001M2.28
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31958-85G2
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