發布時間: 2014 May 25 1217 UTC
Active (M-class flares expected, probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 25 May 2014 | 120 | 007 |
| 26 May 2014 | 122 | 016 |
| 27 May 2014 | 122 | 007 |
There were five C flares and an M flare during the past 24 hours, all released by NOAA AR 12065. The long duration M1.3 flare peaked at 18:35 UT on May 24. No Earth-directed CMEs were observed. STEREO COR2 B imagery registered a CME at 23:09 UT on May 24, but this CME was probably associated to a backside event. In the next 48 hours, the probability for C flares is very high (95%) and for M flares around 60%, especially from NOAA AR 12065. Over the last 24 hours, the solar wind speed as observed by ACE decreased from around 450 km/s to about 430 km/s. Meanwhile the magnitude of the Interplanetary Magnetic Field (IMF) varied between 2 and 4 nT. Over the last 24 hours, geomagnetic conditions were quiet (K Dourbes between 1 and 3; NOAA Kp between 1 and 2). Quiet geomagnetic levels (K Dourbes < 4) are expected on May 25 and 27. Quiet geomagnetic conditions with active (K Dourbes = 4) periods are possible on May 26, due to the expected arrival of a coronal hole high speed stream.
今日估計的國際太陽黑子數(ISN):074,基於13個觀測站。
| 卡塔尼亞沃爾夫數 | /// |
| 10厘米太陽通量 | 118 |
| AK Chambon La Forêt | 012 |
| AK Wingst | 006 |
| 估計地磁Ap指數 | 006 |
| 估計國際太陽黑子數 | 081 - 基於23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 |
|---|---|---|---|---|---|---|---|---|---|
| 24 | 1826 | 1835 | 1844 | ---- | M1.3 | 229 | 53/2065 |
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