發布時間: 2013 Aug 21 1240 UTC
Eruptive (C-class flares expected, probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 21 Aug 2013 | 135 | 018 |
| 22 Aug 2013 | 138 | 008 |
| 23 Aug 2013 | 138 | 003 |
Solar activity was eruptive with a C2.2 flare as strongest flare originating from NOAA AR 1828. A faint partial halo CME was observed in LASCO/C2 around 5h00 UT which was confirmed by STEREO A and B data. It seems to be associated to a small filament eruption located near S15E15, observed in PROBA2/SWAP and GONG H-alpha data. The CME seems to be travelling mainly to the east with a projected speed of 360 km/s. First analysis suggests a possible arrival at 25 August at 9h UT, but this will be further evaluated. We expect C-class flaring activity to continue. There is a slight chance for M-class flares, especially from NOAA active regions 1820 and 1827 that currently have a beta-gamma configuration of their photospheric magnetic field. ACE has observed a jump yesterday at 22h UT in all the plasma parameters jump, but not the magnetic field. This seems to be the arrival of the equatorial CH fast speed stream. Local K-index at Dourbes currently is at K=3 and Kp went up to Kp=4, due to combined effects of the fast speed stream and some influence of a flank of the CME of August 17, that possibly arrived at 2h this morning. Unsettled geomagnetic conditions are expected to continue and return to quiet after 24 hours.
今日估計的國際太陽黑子數(ISN):095,基於13個觀測站。
| 卡塔尼亞沃爾夫數 | /// |
| 10厘米太陽通量 | 132 |
| AK Chambon La Forêt | 012 |
| AK Wingst | 004 |
| 估計地磁Ap指數 | 004 |
| 估計國際太陽黑子數 | 086 - 基於21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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