發布時間: 2021 Oct 08 1232 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 08 Oct 2021 | 081 | 004 |
| 09 Oct 2021 | 081 | 006 |
| 10 Oct 2021 | 081 | 007 |
One sunspots group is visible on the solar surface seen from Earth (Catania sunspots group 58, NOAA AR-2882). The Catania sunspots group 54, NOAA AR-2880 has completely decayed. The Catania sunspot group 58 (NOAA AR-2882) remained magnetically complex (alpha-beta) over the past 24 hours and it produced a C1.9-class flare on Oct 8 peaking at 11:08 UTC. A C.1.1-class flare was also observed near an active region (latitude 33 degree south, and longitude 71 degree east) on Oct 7 around 22:31 UTC, this region does not show any sunspot on the solar surface. More C-class flares are expected with a very small chance of M-class flare.
No Earth directed Coronal Mass Ejection (CME) has been observed in the available coronagraph imagery.
The greater than 10 MeV proton flux was at nominal levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours. The greater than 2 MeV electron flux was below the 1000 pfu and at nominal levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours. The greater than 2 MeV electron fluence was at nominal levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours.
The Earth remained under the slow solar wind speed regime (ranging between 280 km/s and 333 km/) over the past 24 hours. The solar wind parameters (as observed by ACE and DSCOVR) showed an ambient background solar wind flow with interplanetary magnetic field magnitude values returning below 4.0 nT and its Bz components fluctuating between -3.3 nT and 1.3 nT. Nominal solar wind regime is expected to persist in the next 24 hours.
The geomagnetic conditions were quiet over the past 24 hours: Values of K-Dourbes and NOAA-Kp index between 0 and 2 were registered. Quiet conditions are expected to remain as long as the Earth remains in slow solar wind speed regime.
今日估計的國際太陽黑子數(ISN):018,基於22個觀測站。
| 卡塔尼亞沃爾夫數 | 024 |
| 10厘米太陽通量 | 086 |
| AK Chambon La Forêt | 008 |
| AK Wingst | 004 |
| 估計地磁Ap指數 | 004 |
| 估計國際太陽黑子數 | 015 - 基於26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 | |
|---|---|---|---|---|---|---|---|---|---|---|
| 無 | ||||||||||
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 | 21/12/2025 | M1.3 |
| 上一個 地球磁爆 | 21/12/2025 | 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 | 116.9 +25.1 |
| 過去 30 天內 | 109 +22.2 |