發布時間: 2021 Sep 29 1231 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 29 Sep 2021 | 089 | 007 |
| 30 Sep 2021 | 091 | 007 |
| 01 Oct 2021 | 093 | 014 |
Four active regions (ARs) present on the visible solar disk. NOAA AR 2871 has decayed from beta-gamma magnetic field configuration, to alpha. Two new ARs: NOAA AR 2880 (beta) and 2881 (alpha). The former produced a C1.3 flare peaking at 02:18 UT. There’s also a new region rotating into view. Over the next 24 hours, more C-class flares can be expected.
No Earth directed CMEs have been observed in the last 24 hours.
The greater than 10 MeV proton flux was at background levels in the past 24 hours, and is expected to stay there in the next 24 hours. The greater than 2 MeV electron flux remained below the 1000 pfu alert threshold, it may increase over the next 24 hours. The electron fluence was at normal levels over the past 24 hours, it may increase over the next 24 hours.
The Earth is still inside the high speed solar wind from the low latitudinal extension of the northern polar coronal hole (positive polarity). Solar wind speeds have reached 550 km/s with magnetic fields up to 6 nT (with Bz up to -3 nT). Over the next 24 hours we expect a return to slow solar wind.
Geomagnetic conditions were quiet to unsettled for Kp (NOAA Kp 1-3) and reached active periods locally at Dourbes (K Dourbes 2-4) over the past 24 hours, quiet to unsettled conditions can be expected for the next 24 hours. An ICME is expected to arrive after 24 hours and produce active to moderate storm levels.
今日估計的國際太陽黑子數(ISN):074,基於12個觀測站。
| 卡塔尼亞沃爾夫數 | 075 |
| 10厘米太陽通量 | 089 |
| AK Chambon La Forêt | 017 |
| AK Wingst | 013 |
| 估計地磁Ap指數 | 012 |
| 估計國際太陽黑子數 | 055 - 基於23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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