The Sun is full of surprises. Just when you least expect it she produces two M-class solar flares: M1.1 at 18:37 UTC and a very long duration M2.2 solar flare that peaked around at 21:26 UTC.
Solar activty has been very low now for a couple of days. There are only three numbered sunspot regions on the earth-facing solar disk and non of them are likely to produce a strong solar flare. That said, we do not need solar flares and coronal mass ejections for enhanced geomagnetic conditions at Earth. Coronal holes can do the same thing and the effects of such a coronal hole high speed stream is exactly what we are experiencing right now! Image: Aurora Borealis captured by Gibfoto from Tromsø, Norway.
有非常多網友來到SpaceWeatherLive追蹤太陽活動,或確認是否能看見極光,但隨著網站流量增長,維持伺服器的費用也越來越高。如果你喜愛SpaceWeatherLive,可以考慮捐贈維護費用,如此我們可以一起讓網站持續上線!
上一個 X-閃焰 | 01/06/2024 | X1.03 |
上一個 M-閃焰 | 02/06/2024 | M1.9 |
上一個 地球磁爆 | 17/05/2024 | Kp6 (G2) |
無黑子天數 | |
---|---|
上一個無黑子日 | 08/06/2022 |
黑子數月平均 | |
---|---|
4月 2024 | 136.5 +31.6 |
6月 2024 | 194 +57.5 |
Last 30 days | 151 +2.5 |