發布時間: 2026 Jun 25 1231 UTC
C-class flares expected, (probability >=50%)
Minor storm expected (A>=30 or K=5)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 25 Jun 2026 | 141 | 040 |
| 26 Jun 2026 | 140 | 028 |
| 27 Jun 2026 | 138 | 024 |
Solar flaring activity was low over the past 24 hours, with only C-class flares. The largest flare was a C4.3 flare (SIDC Flare 8016) peaking on June 25 at 00:22 UTC, which was produced by SIDC Sunspot Group 902 (NOAA Active Region 4478). A total of 8 numbered sunspot groups were identified on the disk over the past 24 hours. SIDC Sunspot Group 899 (NOAA Active Region 4475) has the most complex magnetic configuration (Beta-Gamma). SIDC Sunspot Group 899 (NOAA Active Region 4475) and SIDC Sunspot Group 902 (NOAA Active Region 4478) are in charge of the majority of the flaring activity of the past 24 hours. 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.
No new Earth-directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph images.
The northern mid latitude negative polarity SIDC Coronal Hole 142 just finished crossing central meridian.
The solar wind parameters became slightly disturbed, following the arrival of the high speed stream. The solar wind speed around 700 km/s and an interplanetary magnetic field of 7nT, and BZ reaching a maximum negative value of -9nT. Similar conditions can be expected for the next 24 hours.
Geomagnetic conditions active to minor storm levels globally and unsettled to active at local levels (Kp up to 5, K_Dourbes up to 4). Active to minor storm conditions can be expected for the next 24 hours, under the continued influence of high speed stream.
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 remained below the 1000 pfu alert threshold, and is expected to remain below the threshold during the next 24 hours. The 24h 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):094,基於22個觀測站。
| 卡塔尼亞沃爾夫數 | 144 |
| 10厘米太陽通量 | 137 |
| AK Chambon La Forêt | 033 |
| AK Wingst | 020 |
| 估計地磁Ap指數 | 020 |
| 估計國際太陽黑子數 | 098 - 基於31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 | 03/06/2026 | X1.0 |
| 上一個 M-閃焰 | 21/06/2026 | M6.9 |
| 上一個 地球磁爆 | 25/06/2026 | Kp5 (G1) |
| 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 | |
|---|---|
| 5月 2026 | 101.4 +22.1 |
| 6月 2026 | 100.5 -0.9 |
| 過去 30 天內 | 103.1 +3.9 |