發布時間: 2023 Dec 10 1236 UTC
M-class flares expected (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 10 Dec 2023 | 126 | 007 |
| 11 Dec 2023 | 126 | 007 |
| 12 Dec 2023 | 126 | 007 |
Solar flaring activity was moderate over past 24 hours with two M-class flares and several C-class flares. The two M1.0 and M2.3 class flares were produced by the complex region, NOAA 3511, with a beta-gamma magnetic class. The flares peak time were at 13:19 UTC on December 09, and at 03:53 UTC on December 10 respectively. This region also produced several C-class flares. The other region, NOAA 3510 and NOAA 3513 also produced several C-class flares. C-class flares are expected in the next 24 hours with some chances of M-class flare from the two beta-gamma magnetic class regions: NOAA 3511 and NOAA 3513.
No Earth directed coronal mass ejection was identified in the currently available SOHO/LASCO-C2 coronographe images.
The mid-latitude south coronal hole with a positive magnetic polarity has crossed the central median. A new equatorial coronal holes with positive magnetic polarity is on the East side of the solar disc facing Earth.
The Solar Wind (SW) conditions near Earth continue to show a slow solar wind regime. The SW speed ranged between 370 km/s and 460 km/s, the total interplanetary magnetic field (Bt) was below 5.0 nT. The North- South magnetic component (Bz) ranged between -4.2 nT and 3.5 nT. The interplanetary magnetic field phi angle was negative (directed towards the Sun) during the past 24 hours. The mid-latitude south coronal hole with a positive magnetic polarity that has crossed the central median on December 07 may slightly affect the SW conditions in the next days. Globally we do expect that the SW conditions remain mostly in a slow solar wind regime in the next 24 hours.
Geomagnetic conditions were quiet both globally and locally (NOAA-Kp and K-BEL 1 to 2) during the last 24 hours. We expect mainly quiet conditions in the next 24 hours in response to the slow solar wind conditions.
The greater than 10 MeV proton flux was at nominal levels 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 the GOES-16 satellite, was ranging around the 1000 pfu alert threshold during the last 24 hours due to the past fast solar wind conditions. It is expected to remain close to 1000 pfu during the next 24 hours. The 24h electron fluence was at moderate levels during the past 24 hours and is expected to remain at these levels for the following 24 hours.
今日估計的國際太陽黑子數(ISN):128,基於08個觀測站。
| 卡塔尼亞沃爾夫數 | /// |
| 10厘米太陽通量 | 128 |
| AK Chambon La Forêt | 005 |
| AK Wingst | 001 |
| 估計地磁Ap指數 | 002 |
| 估計國際太陽黑子數 | 141 - 基於07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 |
|---|---|---|---|---|---|---|---|---|---|
| 09 | 1303 | 1319 | 1337 | ---- | M1.0 | 79/3511 | III/1 | ||
| 10 | 0342 | 0353 | 0358 | S20W66 | M2.3 | SF | 79/3511 |
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 | 12/12/2025 | M1.1 |
| 上一個 地球磁爆 | 12/12/2025 | Kp5 (G1) |
| 無黑子天數 | |
|---|---|
| 上一個無黑子日 | 08/06/2022 |
| 黑子數月平均 | |
|---|---|
| 11月 2025 | 91.8 -22.8 |
| 12月 2025 | 131.8 +40 |
| 過去 30 天內 | 109.8 +17.3 |