發布時間: 2023 Mar 16 1231 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 16 Mar 2023 | 138 | 019 |
| 17 Mar 2023 | 136 | 011 |
| 18 Mar 2023 | 134 | 008 |
The solar flaring activity remained at low levels over the past 24 hours. Only two C-class flares were detected: C1.0 flare peaking at 22:16 UTC on March 15 and C1.3 flare peaking at 06:43 UTC on March 16, both associated with unnumbered active region near N23W21. As there are no complex active regions observed on the visible side of the solar disk, the flaring activity is expected to continue at very low to low levels over the next 24 hours with isolated C-class flaring.
During last 24 hours there were no potentially Earth-directed CMEs detected in the available coronagraph observations.
The greater than 10 MeV proton has returned to near the nominal levels in the past 24 hours. The proton flux is expected to be at the nominal levels over the next day. The greater than 2 MeV electron flux has been below the 1000 pfu threshold and is expected to remain so. The 24h electron fluence was at nominal levels and is expected to remain so over the next 24 hours.
An equatorial coronal hole of positive polarity started to transit the central meridian this morning and is expected to influence solar wind conditions starting late March 19.
Solar wind parameters were slightly elevated due to the influence of the high-speed stream coming from coronal hole (positive polarity) and ICME. The solar wind speed values were between 480 km/s and 580 km/s. The interplanetary magnetic field magnitude ranged between 4 nT and 13 nT. The southward component of the interplanetary magnetic field fluctuated between -12 nT and 13 nT. The solar wind speed is expected to continue to be elevated in the next 24 hours due to the combination of the possible arrival of glancing blow of CME from the filament eruption observed on March 13, and ongoing influence of the HSS, with gradually decrease over the next days, as the influence of the HSS begins to wane.
Geomagnetic conditions were quiet to active both globally and locally (K-Bel=1-4 NOAA-Kp=1-4) with isolated moderate storm period globally (NOAA- Kp = 6) and minor storm period locally (K Belgium reaching 5) at around 21:00 UTC on March 15. Geomagnetic conditions are expected to be quiet to active in the next days, with a chance of isolated minor storm periods during next days due to influence of the HSS and possible glancing blow from the CMEs.
今日估計的國際太陽黑子數(ISN):097,基於15個觀測站。
| 卡塔尼亞沃爾夫數 | 135 |
| 10厘米太陽通量 | 136 |
| AK Chambon La Forêt | 027 |
| AK Wingst | 028 |
| 估計地磁Ap指數 | 027 |
| 估計國際太陽黑子數 | 106 - 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 | 04/02/2026 | X4.21 |
| 上一個 M-閃焰 | 25/02/2026 | M2.4 |
| 上一個 地球磁爆 | 03/03/2026 | Kp5 (G1) |
| 無黑子天數 | |
|---|---|
| 過去 365 天內 | 3天 |
| 2026 | 3天 (5%) |
| 上一個無黑子日 | 24/02/2026 |
| 黑子數月平均 | |
|---|---|
| 2月 2026 | 78.2 -34.3 |
| 3月 2026 | 75 -3.2 |
| 過去 30 天內 | 56.5 -68.4 |