發布時間: 2023 Jan 23 1303 UTC
M-class flares expected (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 23 Jan 2023 | 200 | 007 |
| 24 Jan 2023 | 198 | 007 |
| 25 Jan 2023 | 196 | 017 |
Solar flaring activity was moderate and frequent, with two M1 and numerous C-class flares detected during the past 24 hours. NOAA Active Region (AR) 3190 (magnetic type Beta-Gamma-Delta, Catania group 48) emitted the first M1 flare yesterday at 12:26 UT, while NOAA AR 3194 (magnetic type Beta-Gamma-Delta, Catania group 46) produced the second M1 yesterday at 17:02 UT. NOAA AR 3194 is likely to produce isolated M-class events and there is a chance for NOAA AR 3190 to reach the same level of flare activity in the next 24 hours. NOAA AR 3191 (magnetic type Beta, Catania group 47), 3192 (magnetic type Beta-Gamma, Catania group 49), 3199 (magnetic type Beta, Catania group 55), and 3200 (magnetic type Beta) have complex magnetic configurations, produced numerous C-class flares and are expected to remain at the C-class activity level in the next 24 hours.
No Earth-directed Coronal Mass Ejections were observed in the last 24 hours.
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 remained below the 1000 pfu alert threshold and is expected to remain below this threshold during the next 24 hours. The 24h electron fluence was at nominal levels and is expected to remain so.
The Solar Wind (SW) conditions remained slightly disturbed. The SW speed fluctuated between 420 to 570 km/s, while the total magnetic field (Bt) varied between 5 and 12 nT, and its North-South (Bz) component ranged between -8 and 12 nT in the last 24 hours. The interplanetary magnetic field phi angle was most of the time directed away from the Sun over the last 24 hours. The current SW conditions may have been the result of a glancing blow that arrived today at 03:00 UT. As such the SW conditions are expected to continue with the same pattern in the next 24 hours.
Geomagnetic conditions were quiet both globally and locally (NOAA Kp 1-3 and K Belgium 0-3) over the last 24 hours. The are expected to remain at the same level, and perhaps increase to moderate levels for a short period of time, for the next 24 hours.
今日估計的國際太陽黑子數(ISN):169,基於02個觀測站。
| 卡塔尼亞沃爾夫數 | /// |
| 10厘米太陽通量 | 199 |
| AK Chambon La Forêt | 015 |
| AK Wingst | 010 |
| 估計地磁Ap指數 | 010 |
| 估計國際太陽黑子數 | 164 - 基於10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 |
|---|---|---|---|---|---|---|---|---|---|
| 22 | 1212 | 1226 | 1234 | ---- | M1.1 | 48/3190 | |||
| 22 | 1649 | 1702 | 1710 | S26W51 | M1.6 | 1B | 46/3194 |
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 | 125.7 +33.9 |
| 過去 30 天內 | 109.3 +18.1 |