發布時間: 2026 Apr 22 1231 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 22 Apr 2026 | 118 | 008 |
| 23 Apr 2026 | 122 | 008 |
| 24 Apr 2026 | 126 | 007 |
Solar flaring activity was low over the past 24 hours, with only C-class flares identified. A total of 4 numbered sunspot groups were identified on the disk over the past 24 hours. SIDC Sunspot Group 825 (NOAA Active Region 4419) and SIDC Sunspot Group 847 (NOAA Active Region 4420) are the largest and most magnetically complex (Beta-Gamma) regions on disk. The largest flare was a C1.9 flare (SIDC Flare 7436) peaking on April 21 at 14:24 UTC, which was produced by SIDC Sunspot Group 847. Solar flaring activity is expected to be low over the next 24 hours, with C-class flares very likely and a chance for M-class flares.
A Coronal Mass Ejection (CME) was observed LASCO-C2 data around 23:00 UTC on April 20. This CME is associated with a filament eruption centred around N21, E05, with a speed around 430 km/s. The bulk of the material is expected to travel North and most likely to miss the Earth a glancing blow arrival is possible on April 25 around 09:00 UTC.
SIDC Coronal Hole 157 (equatorial coronal hole extending to the polar south with a positive polarity) is continuing to cross the central meridian. SIDC Coronal Hole 156 (equatorial coronal hole with a positive polarity) started crossing the central meridian on April 22.
Over the past 24 hours the solar wind parameters were under the waning influence of a high-speed stream associated with SIDC Coronal Hole 147. The solar wind speed ranged between 474 km/s to 577 km /s. The total interplanetary magnetic field ranged from 3 to 6 nT, with the Bz reaching a minimum of -5 nT. The phi-angle was mainly in the negative sector (directed towards the Sun), with periods in the positive sector. Quite solar wind conditions are expected in the next 24 hours.
The geomagnetic conditions reached active conditions globally (Kp 4) and minor storm conditions locally (K BEL 5) in the last 24 hours. Quiet to unsettled conditions are expected over the next 24 hours.
The greater than 10 MeV GOES proton flux was at background levels and is expected to remain at background levels over the next 24 hours.
The greater than 2 MeV electron flux, as measured by GOES-18 and GOES-19 was 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 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):075,基於21個觀測站。
| 卡塔尼亞沃爾夫數 | 079 |
| 10厘米太陽通量 | 112 |
| AK Chambon La Forêt | 020 |
| AK Wingst | 022 |
| 估計地磁Ap指數 | 021 |
| 估計國際太陽黑子數 | 056 - 基於32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 | 91.5 +12.2 |
| 過去 30 天內 | 96.4 +4.5 |