發布時間: 2013 Apr 13 1248 UTC
Active (M-class flares expected, probability >= 50%)
Severe geomagnetic storm expected (A>=100 or K>=7)
Warning condition
| 10公分通量 | Ap | |
|---|---|---|
| 13 Apr 2013 | 140 | 039 |
| 14 Apr 2013 | 142 | 045 |
| 15 Apr 2013 | 143 | 008 |
Catania sunspot groups 40 and 43 (NOAA ARs 1718 and 1719 respectively) show the signs of decay, although these two active regions (as well as Catania sunspot group 45, NOAA AR 1721) have beta-gamma configuration of the photospheric magnetic field. M3.3 flare was detected on April 12 peaking at 20:38 UT in the Catania sunspot group 40 (NOAA AR 1718). It was not associated with a CME. The delta sunspot in the Catania sunspot group 43 (NOAA AR 1719) does not exist anymore, so an X-flare (and an SEP event) is not very likely (although an Earth-directed CME remains possible). We expect further flaring activity on the M-level, with a non-negligible chance for an isolated X-class flare. The proton flux at energies above 10 MeV is currently below the SEP event threshold, although it still exceeds significantly the background level. In such a situation, a relatively small increase of the proton flux at the expected shock arrival may lead to crossing the SEP event threshold again. The Earth is currently inside a slow (around 400 km/s) solar wind flow with average (around 4 nT) interplanetary magnetic field magnitude. We expect quiet geomagnetic conditions until the arrival (expected later today) of the interplanetary disturbance produced by the halo CME of April 11. The occurrence of a strong geomagnetic storm (K index around 7) will be probable.
今日估計的國際太陽黑子數(ISN):080,基於13個觀測站。
| 卡塔尼亞沃爾夫數 | 125 |
| 10厘米太陽通量 | 138 |
| AK Chambon La Forêt | 010 |
| AK Wingst | 005 |
| 估計地磁Ap指數 | 004 |
| 估計國際太陽黑子數 | 081 - 基於20個觀測站 |
| 日 | 開始 | 最大值 | 結束 | 位置 | 強度 | OP | 10cm | 電波爆發類型 | 卡塔尼亞天體物理觀測站/美國國家海洋暨大氣管理局 |
|---|---|---|---|---|---|---|---|---|---|
| 12 | 1952 | 2038 | 2046 | N21W42 | M3.3 | 40/1718 |
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