發布時間: 2022 Feb 25 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 | |
|---|---|---|
| 25 Feb 2022 | 093 | 009 |
| 26 Feb 2022 | 095 | 015 |
| 27 Feb 2022 | 097 | 015 |
The Sun produced no C flares in the past 24 hours. The chance for a C flare in the next 24 hours is estimated at 40%.
No Earth-directed Coronal Mass Ejections (CMEs) were observed in available coronagraphic imagery.
The greater than 10 MeV proton flux was at nominal levels in the past 24 hours, and is expected to stay at nominal levels in the next 24 hours. The greater than 2 MeV electron flux exceeded the 1000 pfu threshold in the past 24 hours, and may exceed that threshold again in the next 24 hours. The greater than 2 MeV electron fluence was at nominal levels in the past 24 hours, and may reach moderate levels in the next 24 hours.
The solar wind speed as registered by DSCOVR varied between about 380 and 490 km/s in the past 24 hours, with current values near 445 km/s. The magnitude of the Interplanetary Magnetic Field near Earth (IMF) varied between about 0 and 8 nT, and its orientation was predominantly away from the Sun. There were no extended time intervals with Bz below -5 nT. A further decrease of solar wind conditions is expected on February 25. On February 26 and 27, enhanced solar wind levels are possible due to the expected arrival of a high speed stream from a positive polarity equatorial coronal hole.
Quiet geomagnetic conditions (K-BEL between 1 and 2; NOAA Kp between 0 and 3) were registered in the past 24 hours. Quiet to unsettled geomagnetic levels (K-BEL < 4) are expected on February 25, with a chance for active intervals (K-BEL = 4). Active intervals are possible on February 26 and 27, with a slight chance for minor storm intervals (K-BEL = 5), due to the expected arrival of a high speed stream from a positive polarity equatorial coronal hole.
今日估計的國際太陽黑子數(ISN):022,基於17個觀測站。
| 卡塔尼亞沃爾夫數 | /// |
| 10厘米太陽通量 | 092 |
| AK Chambon La Forêt | 009 |
| AK Wingst | 007 |
| 估計地磁Ap指數 | 007 |
| 估計國際太陽黑子數 | 036 - 基於18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 | ||||||||||
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