發布時間: 2021 Dec 14 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Active conditions expected (A>=20 or K=4)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 14 Dec 2021 | 081 | 009 |
| 15 Dec 2021 | 082 | 016 |
| 16 Dec 2021 | 082 | 010 |
Regions Catania 82, Catania 83/NOAA 2905, NOAA 2906 and Catania 84/NOAA 2907 are present on the visible solar disk. Region Catania 84 was the source of a C1.4-class flare recorded by GOES on Dec 14 08:36UT. C class flares are possible over the next 24 hours.
No Earth directed CMEs were observed in the past 24 hours.
The greater than 10 MeV proton flux was at nominal levels in the past 24 hours and is expected to remain at nominal levels in 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 level during the next 24 hours. The greater than 2 MeV electron fluence was at nominal levels in the past 24 hours and is expected remain so in the next 24 hours.
Over the past 24 hours, the solar wind parameters (ACE+DSCOVR) remained in the slow regime. The expected high-speed stream (HSS) emanating from the small equatorial negative polarity Coronal Hole (CH) that appeared on Dec 12 seems to have not had an impact yet. A southern negative polarity CH crossed central meridian on Dec 13. Its effects can be expected about Dec 15-16. The total magnetic field reached 8 nT, and its southward component, Bz, fluctuated between -6 nT and +7 nT in the past 24 hours. The solar wind speed had values ranging from 300 km/s to 335 km/s. The interplanetary magnetic field phi angle has been varied since about Dec 13 19:00UT. Over the next 24 hours, we are expecting slight enhacements due to the effects afore mentioned HSS.
Geomagnetic conditions were quiet tover the past 24 hours (NOAA Kp and K-BEL recorded values 0-2). Geomagnetic conditions are expected to remain mostly quiet over the next 24 hours with some unsettled periods in response to the influence of the wind stream associated with the small equatorial coronal hole.
今日估計的國際太陽黑子數(ISN):037,基於07個觀測站。
| 卡塔尼亞沃爾夫數 | 035 |
| 10厘米太陽通量 | 081 |
| AK Chambon La Forêt | 008 |
| AK Wingst | 005 |
| 估計地磁Ap指數 | 004 |
| 估計國際太陽黑子數 | 022 - 基於13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 | 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 | 106.7 -17.3 |
| 過去 30 天內 | 102.5 -7.3 |