發布時間: 2024 Dec 20 1232 UTC
M-class flares expected (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 20 Dec 2024 | 179 | 007 |
| 21 Dec 2024 | 181 | 007 |
| 22 Dec 2024 | 193 | 007 |
A total of 6 numbered sunspot groups were identified on the disk over the past 24 hours. There have been four M-class flares in the last 24 hours. The largest one was an M3.8 flare peaking at 15:34 UTC on 19 December, coming from SIDC Sunspot Group 323 (NOAA Active Region 3928, beta magnetic field configuration). The other M-class flares came from the same AR and one from SIDC Sunspot Group 337 (NOAA Active Region 3924, beta gamma magnetic field configuration), which is rotating out of view over the west limb. More M-class flares can be expected and X-flares are possible in the next 24 hours.
A full halo CME was observed at 18:16 UTC on 19 December by LASCO C3 (after a data gap of several hours). The source of this CME is believed to be backsided and will thus not arrive to the Earth.
The solar wind at Earth has a speed around 460 km/s and interplanetary magnetic field around 8 nT (DSCOVR). Similar conditions are expected to persist in the next 24 hours. The CME from 15 December may still arrive today, but it has probably missed the Earth.
Geomagnetic conditions have reached active levels both globally and locally (Kp and K_Bel up to 4). Mostly quiet to unsettled conditions expected for the next 24 hours. The CME from 15 December may still arrive today and create disturbed conditions, but it has probably missed the Earth.
The greater than 10 MeV proton flux was below the threshold level over the past 24 hours. It is expected to remain below the threshold level over the next 24 hours.
The greater than 2 MeV electron flux measured by GOES 16 and GOES 18 remained below the threshold level in the last 24 hours. It is expected to remain so over the next 24 hours. The 24-hour electron fluence is presently at normal levels and is expected to remain so over the next 24 hours.
今日估計的國際太陽黑子數(ISN):152,基於13個觀測站。
| 卡塔尼亞沃爾夫數 | 117 |
| 10厘米太陽通量 | 175 |
| AK Chambon La Forêt | 016 |
| AK Wingst | 014 |
| 估計地磁Ap指數 | 012 |
| 估計國際太陽黑子數 | 121 - 基於09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 |
|---|---|---|---|---|---|---|---|---|---|
| 19 | 1021 | 1038 | 1057 | S19W72 | M1.6 | SF | 50/3924 | ||
| 19 | 1527 | 1534 | 1539 | ---- | M3.8 | --/3928 | |||
| 19 | 1856 | 1900 | 1904 | ---- | M1.7 | --/3928 | |||
| 20 | 0720 | 0726 | 0735 | ---- | M2.1 | 50/3924 | |||
| 20 | 1115 | 1118 | 1122 | ---- | M2.5 | 59/3928 |
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 | 08/12/2025 | X1.1 |
| 上一個 M-閃焰 | 31/12/2025 | M7.11 |
| 上一個 地球磁爆 | 02/01/2026 | Kp5 (G1) |
| 無黑子天數 | |
|---|---|
| 上一個無黑子日 | 08/06/2022 |
| 黑子數月平均 | |
|---|---|
| 12月 2025 | 124 +32.2 |
| 1月 2026 | 110 -14 |
| 過去 30 天內 | 104.3 -5.3 |