發布時間: 2014 Nov 03 1244 UTC
Eruptive (C-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Warning condition (activity levels expected to increase, but no numeric forecast given)
| 10公分通量 | Ap | |
|---|---|---|
| 03 Nov 2014 | 128 | 011 |
| 04 Nov 2014 | 132 | 011 |
| 05 Nov 2014 | 136 | 007 |
Solar flaring activity was dominated by a yet unnumbered region currently turning around the East limb. It produced the two largest flares of the period: a C9.4 flare peaking at 21:05 UT and an M2.2 flare peaking around 11:53 UT. Four C flares (all below C5) originated from Catania group 3 (NOAA AR 2201). NOAA AR 2203 grew in size and new sunspot emergence was observed in NOAA plage region 2197 (previous Catania group 97). Flaring at C level is expected to continue and M flares remain possible from the new region turning around the East limb. No Earth directed CME's were observed during the period. The >10 MeV proton flux as observed by GOES passed the event threshold a number of times for very short periods (5 to 10 minutes) at 21:10UT-21:15UT, 22:10UT-22:15UT, 22:30UT-22:40UT and 22:45UT-22:50UT. The proton flux remained below 11 pfu. The proton flux has been increasing and decreasing several times since November 1 at 14:30 UT. The sequence of several rises indicates the relation with several solar events. Further increases of the proton flux and in the next 24 hours are likely, with chances for a stronger proton event. Solar wind speed decreased during the period from close to 500 km/s after the start of the period to around 420 km/s currently. The total magnetic field also decreased from within the 3-7 nT range to the 1-4nT range, with the z-component not reaching below -4nT. Phi angle was variable. Geomagnetic conditions were quiet to unsettled (both NOAA Kp and local K Dourbes 1-3). Under the influence of a coronal hole high speed stream, solar wind conditions may become slightly elevated in the next 24 to 48 hours with associated unsettled and possibly active geomagnetic conditions.
今日估計的國際太陽黑子數(ISN):086,基於11個觀測站。
| 卡塔尼亞沃爾夫數 | /// |
| 10厘米太陽通量 | 124 |
| AK Chambon La Forêt | 014 |
| AK Wingst | 008 |
| 估計地磁Ap指數 | 008 |
| 估計國際太陽黑子數 | 070 - 基於24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 |
|---|---|---|---|---|---|---|---|---|---|
| 03 | 1123 | 1153 | 1217 | ---- | M2.2 | --/---- | II/2 |
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