發布時間: 2023 Oct 26 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 26 Oct 2023 | 127 | 014 |
| 27 Oct 2023 | 129 | 015 |
| 28 Oct 2023 | 129 | 010 |
The solar flaring activity was at low levels, with several C-class flares recorded in the past 24 hours. There are currently only two numbered active regions on the solar disk with sunspots remaining. The largest flare was an C3.0 flare, peaking at 22:44 on Oct 25, associated with NOAA AR 3471 (beta class). NOAA AR 3468 (alpha class) did not show any significant flaring activity. The solar flaring activity is expected to be at low levels over the next 24 hours with a C-class flares possible.
No Earth directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph imagery.
Over the past 24 hours, the solar wind conditions became slightly disturbed with the total interplanetary magnetic field rose to 13 nT at around 08:30 UTC on 26 Oct. The southward component of the interplanetary magnetic field ranged between -12 nT and 8 nT. The solar wind speed followed an increasing trend, rising from 310 km/s to 380 km/s. The magnetic field orientation was variable at the start of the period before switching to the predominantly positive sector (field directed away from the Sun) from 19:30 UTC on Oct 25. This might be associated with arrival of the compression region in front of the expected HSS from a positive polarity coronal hole. Solar wind parameters are expected to remain slightly elevated in the next days due to HSS arrival associated with the positive polarity coronal hole, that transited the central meridian on Oct 23.
Geomagnetic conditions over the past 24 hours were quiet to unsettled (NOAA Kp: 1 to 3 and K-BEL: 1 to 3). Geomagnetic conditions are expected to be at quiet to unsettled levels with a chance for isolated active and minor storm periods in response to the high-speed stream arrival from a positive polarity coronal hole.
Over the past 24 hours the greater than 10 MeV GOES proton flux was at nominal levels and is expected to remain so over the next days.
The greater than 2 MeV electron flux remained below the 1000 pfu threshold as measured by GOES 16. It is expected to remain below this threshold over the next days. The 24 hour 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):052,基於14個觀測站。
| 卡塔尼亞沃爾夫數 | /// |
| 10厘米太陽通量 | 126 |
| AK Chambon La Forêt | 009 |
| AK Wingst | 003 |
| 估計地磁Ap指數 | 002 |
| 估計國際太陽黑子數 | 031 - 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 | |
|---|---|---|---|---|---|---|---|---|---|---|
| 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 | 30/03/2026 | X1.5 |
| 上一個 M-閃焰 | 04/04/2026 | M1.0 |
| 上一個 地球磁爆 | 03/04/2026 | Kp7- (G3) |
| 無黑子天數 | |
|---|---|
| 過去 365 天內 | 3天 |
| 2026 | 3天 (3%) |
| 上一個無黑子日 | 24/02/2026 |
| 黑子數月平均 | |
|---|---|
| 3月 2026 | 85.9 +7.7 |
| 4月 2026 | 128.3 +42.3 |
| 過去 30 天內 | 97.5 +35.7 |