發布時間: 2024 Oct 15 1231 UTC
M-class flares expected (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 15 Oct 2024 | 181 | 008 |
| 16 Oct 2024 | 175 | 007 |
| 17 Oct 2024 | 170 | 017 |
Solar flaring activity was moderate over the past 24 hours with 3 M-class flares. The largest flare was a M1.9 flare peaking on October 15 at 02:13 UTC, which was produced by SIDC Sunspot Group 283 (NOAA Active Region 3854).There are currently 8 numbered active regions on the visible disk. The most complex regions are SIDC SGs 281 and 283 (NOAA AR 3852 and 3854) all magnetic type beta-gamma. The solar flaring activity is expected to be at moderate levels over the next 24 hours with C-class flares expected and M-class flares probable and a low chance of X-class flares.
No new Earth-directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph images.
A positive polarity mid-latitude coronal hole (SIDC Coronal Hole 68) continues to cross the central meridian. A high-speed stream from this coronal hole may impact the Earth/enhance the solar wind environment near Earth on October 17.
The solar wind at the Earth remained mostly slow over the last 24 hours. The solar wind speed was around 400 km/s and the interplanetary magnetic field was around 7nT. The Bz reached a minimum value of -5 nT. A small shock was observed on October 14 at 17:18 UTC. The interplanetary magnetic field jumped from 6 nT to 9 nT, with the Bz component changing from -2 nT to -4 nT. The solar wind speed jumped from 381 km/s to around 403 km/s. The solar wind density at the shock jumped from 2.62 ppcc to around 6.68 ppcc (ACE). Slow solar wind conditions are expected in the next 24h.
Geomagnetic conditions were globally and locally quiet to active (Kp 4- and K Bel 3). Quiet conditions are expected in the next 24 hours.
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 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):116,基於12個觀測站。
| 卡塔尼亞沃爾夫數 | 161 |
| 10厘米太陽通量 | 182 |
| AK Chambon La Forêt | 018 |
| AK Wingst | 008 |
| 估計地磁Ap指數 | 008 |
| 估計國際太陽黑子數 | 139 - 基於16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 |
|---|---|---|---|---|---|---|---|---|---|
| 14 | 1322 | 1337 | 1350 | ---- | M1.8 | 36/3848 | III/2 | ||
| 15 | 0202 | 0213 | 0223 | S12W21 | M1.9 | SF | 45/3854 | ||
| 15 | 0223 | 0227 | 0231 | S11W23 | M1.1 | 1 | 42/3852 | III/1VI/2 |
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 | 31/12/2025 | M7.11 |
| 上一個 地球磁爆 | 10/01/2026 | Kp6 (G2) |
| 無黑子天數 | |
|---|---|
| 上一個無黑子日 | 08/06/2022 |
| 黑子數月平均 | |
|---|---|
| 12月 2025 | 124 +32.2 |
| 1月 2026 | 106.7 -17.3 |
| 過去 30 天內 | 101.8 -7.7 |