發布時間: 2026 Apr 17 1231 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 17 Apr 2026 | 110 | 007 |
| 18 Apr 2026 | 110 | 007 |
| 19 Apr 2026 | 110 | 007 |
A total of 3 numbered sunspot groups were identified on the disk over the past 24 hours. Solar flaring activity was low over the past 24 hours, with only C-class flares identified. These flares originated at SIDC Sunspot Group 825 (NOAA Active Regions 4397, 4419), currently located at N15E38, with a Beta-Gamma magnetic configuration. The largest flare was a C4.1 flare (SIDC Flare 7416) peaking on April 17 at 04:42 UTC, which was produced by SIDC Sunspot Group 825. More c-class flares can be expected in the next 24 hours, and there are low chances of observing an M-class flare.
No Earth directed CMEs were observed in the past 24 hours.
There is a large equatorial coronal hole with negative polarity in the western hemisphere (SIDC Coronal Hole 147).
The solar wind speed is low, around 310 km/s with interplanetary magnetic field magnitude of 5 nT, with positive polarity (away from the Sun). The high speed solar wind stream from a large coronal hole located in the northern hemisphere (SIDC Coronal Hole 147) will reach the Earth in about 24 hours.
Geomagnetic conditions have been quiet (Kp and K_BEL up to 2). Similar conditions can be expected for the next 24 hours, after that the high speed stream from SIDC Coronal Hole 147 will reach the Earth and create disturbed conditions.
The greater than 10 MeV proton flux, as measured by GOES-18, was below the 10 pfu threshold level over the past 24 hours and is expected to remain so for the next 24 hours.
The greater than 2 MeV electron flux, as measured by GOES-18 and GOES-19 was briefly above the 1000 pfu alert threshold in the past 24 hours. The flux is expected to fluctuate around the alert threshold over the next 24 hours. The 24-hour electron fluence was at normal to moderate levels over the past 24 hours and is expected to remain at these levels over the next 24 hours.
今日估計的國際太陽黑子數(ISN):051,基於20個觀測站。
| 卡塔尼亞沃爾夫數 | /// |
| 10厘米太陽通量 | 108 |
| AK Chambon La Forêt | 006 |
| AK Wingst | 003 |
| 估計地磁Ap指數 | 002 |
| 估計國際太陽黑子數 | 054 - 基於25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 | 24/04/2026 | X2.5 |
| 上一個 M-閃焰 | 22/05/2026 | M2.3 |
| 上一個 地球磁爆 | 16/05/2026 | Kp6- (G2) |
| 無黑子天數 | |
|---|---|
| 過去 365 天內 | 3天 |
| 2026 | 3天 (2%) |
| 上一個無黑子日 | 24/02/2026 |
| 黑子數月平均 | |
|---|---|
| 4月 2026 | 79.3 -6.6 |
| 5月 2026 | 87.5 +8.2 |
| 過去 30 天內 | 95.7 +3.6 |