發布時間: 2015 Oct 12 1230 UTC
C-class flares expected, (probability >=50%)
Minor storm expected (A>=30 or K=5)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 12 Oct 2015 | 089 | 016 |
| 13 Oct 2015 | 093 | 034 |
| 14 Oct 2015 | 097 | 027 |
The 4 sunspot groups currently visible on the solar disk are quiet. An active region (AR) is approaching the east limb and produced the only C-class flare of the period: C3.2 at 22:29UT. No earth-directed coronal mass ejections (CMEs) have been observed.
C-class flares are expected, with a small chance on an M-class flare from the AR just behind the east limb.
Solar wind speed continued its decline to values around 440 km/s until about 07:00UT, when a gradual increase was observed up to its current 500 km/s. Bz oscillated between -7 and +6 nT, with a sustained negative period at around -7nT between 08:00 and 11:00UT. The interplanetary magnetic field (IMF) was mostly directed away from the Sun (positive). Geomagnetic conditions ranged from quiet to unsettled, with a minor storming episode (Kp=5) during the 09-12UT interval. Active episodes were observed at Dourbes shortly before midnight. The high speed wind stream (HSS) from a wide northern coronal hole (CH) is expected to arrive later today and to continue possibly for the next two days.
Unsettled to active geomagnetic conditions are expected, with a good chance on minor geomagnetic storming episodes from the influence of the CH HSS.
今日估計的國際太陽黑子數(ISN):052,基於17個觀測站。
| 卡塔尼亞沃爾夫數 | /// |
| 10厘米太陽通量 | 085 |
| AK Chambon La Forêt | 021 |
| AK Wingst | 020 |
| 估計地磁Ap指數 | 018 |
| 估計國際太陽黑子數 | 027 - 基於19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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