發布時間: 2013 Jul 20 1408 UTC
Eruptive (C-class flares expected, probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 20 Jul 2013 | 114 | 015 |
| 21 Jul 2013 | 113 | 015 |
| 22 Jul 2013 | 113 | 012 |
The only C-class flare reported during the last 24 hours was C2.1 flare originating from the NOAA AR 1793. This active region currently has beta- gamma configuration of the photosperic magnetic field and the potential to produce C-class and possibly M-class flares. The newly arrived data showed that the CME on July 18 associated with the prominence eruption on the east solar limb, is most probably not Earth-directed. The Earth is still inside the fast speed stream due to the low-latitude coronal hole in the northern hemisphere. At the moment the solar wind speed is 530 km/s and the interplanetary magnetic field (IMF) is rather stable with the magnitude of about 2 nT. We expect unsettled to active geomagnetic conditions due to the currently ongoing influence of the fast stream. The arrival of the fast flow from the low-latitude coronal hole (also crossing the equator) in the southern hemisphere, which just reached the central meridian is expected on July 23.
今日估計的國際太陽黑子數(ISN):037,基於12個觀測站。
| 卡塔尼亞沃爾夫數 | /// |
| 10厘米太陽通量 | 114 |
| AK Chambon La Forêt | 023 |
| AK Wingst | 020 |
| 估計地磁Ap指數 | 019 |
| 估計國際太陽黑子數 | 058 - 基於25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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