發布時間: 2024 Oct 20 1231 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 20 Oct 2024 | 161 | 019 |
| 21 Oct 2024 | 165 | 022 |
| 22 Oct 2024 | 165 | 016 |
Solar flaring activity was moderate over the past 24 hours, with 1 M-class flare identified. The largest flare was a M1.7 flare (SIDC Flare 2358) peaking on October 19 at 14:34 UTC, which was produced by SIDC Sunspot Group 283 (NOAA Active Region 3854). A total of 7 numbered sunspot groups were identified on the disk over the past 24 hours. SIDC Sunspot Group 285 and 288 (resp. NOAA Active Region 3856 and 3859) are the most complex (beta-gamma). Solar flaring activity is expected to be low over the next 24 hours, with C-class flares very likely and M-class flares possible.
No new Earth-directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph images.
The solar wind at the Earth is slow. The speeds temporarily increased yesterday evening from around 400 km/s to 470 km/s and is now back around 400 km/s. The interplanetary magnetic field was around 7 nT with the Bz reaching a minimum value of -6 nT. The solar wind speed may become slightly enhanced on 21 OCT, due to the potential arrival of the high-speed stream (HSS).
Geomagnetic conditions were quiet to active globally (NOAA Kp 4) and quiet to minor storm locally (K Belgium 5) over the past 24 hours. Geomagnetic conditions are expected to remain unsettled to active due to a high-speed stream arrival of the Coronal Hole that crossed the central meridian on OCT 18.
The greater than 10 MeV proton flux remained below the 10 pfu threshold and is expected to remain so over the next days.
The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold, and it is expected to remain below the threshold during the next 24 hours. The 24h electron fluence was at normal levels and is expected to remain so.
今日估計的國際太陽黑子數(ISN):122,基於08個觀測站。
| 卡塔尼亞沃爾夫數 | /// |
| 10厘米太陽通量 | 162 |
| AK Chambon La Forêt | 034 |
| AK Wingst | 029 |
| 估計地磁Ap指數 | 031 |
| 估計國際太陽黑子數 | 135 - 基於14個觀測站 |
| 日 | 開始 | 最大值 | 結束 | 位置 | 強度 | OP | 10cm | 卡塔尼亞天體物理觀測站/美國國家海洋暨大氣管理局 | 電波爆發類型 |
|---|---|---|---|---|---|---|---|---|---|
| 19 | 1427 | 1434 | 1440 | ---- | M1.7 | --/3854 |
由太陽影響數據分析中心提供© - SIDC - 由 SpaceWeatherLive處理
所有時間均採用 UTC 時間
很多網友來到 SpaceWeatherLive 追蹤太陽活動或極光觀測機會,但隨著流量增加,維持伺服器運作的成本也隨之越高。若您喜歡 SpaceWeatherLive 並想支持這個計畫,可選擇訂閱無廣告版本,或考慮捐款。有了您的幫助,我們才能讓 SpaceWeatherLive 持續運作!
| 上一個 X-閃焰 | 08/12/2025 | X1.1 |
| 上一個 M-閃焰 | 20/12/2025 | M1.0 |
| 上一個 地球磁爆 | 12/12/2025 | Kp5 (G1) |
| 無黑子天數 | |
|---|---|
| 上一個無黑子日 | 08/06/2022 |
| 黑子數月平均 | |
|---|---|
| 11月 2025 | 91.8 -22.8 |
| 12月 2025 | 118.5 +26.7 |
| 過去 30 天內 | 108.7 +20.4 |