發布時間: 2024 Mar 12 1232 UTC
M-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 | |
|---|---|---|
| 12 Mar 2024 | 127 | 007 |
| 13 Mar 2024 | 125 | 016 |
| 14 Mar 2024 | 123 | 007 |
There are four active regions visible on the solar disk. NOAA AR 3599 is the only one with a complex magnetic field configuration (beta-gamma-delta), and producing most of the recent flaring. The strongest flare was a C3.9, that peaked at 11:35 UTC, from NOAA AR 3599. M-class flares can be expected, X-class flares are possible.
No Earth-directed CMEs were detected in the available coronagraph observations in the last 24 hours.
An equatorial (positive polarity) coronal hole crossed the central meridian on March 10. The high speed solar wind from this coronal hole may arrive at Earth on 13 March.
The Earth is inside slow solar wind, with speeds close to 420 km/s and an interplanetary magnetic field around 5 nT. Similar solar wind conditions can be expected over the next 24 hours. A high speed stream and a glancing blow from the 11 March CME will probably create disturbed conditions in the second half of 13 March.
Geomagnetic conditions were quiet to unsettled (NOAA_Kp up to 3 and K_BEL up to 2). Similar conditions are expected for the next 24 hours. After that, a glancing blow from the 11 March CME and a high speed stream could arrive on 13 March and cause active conditions.
The greater than 10 MeV proton flux was below the threshold level over the past 24 hours and is expected to remain so for the next 24 hours.
The greater than 2 MeV electron flux from GOES 16 was slightly above the threshold level in the last 24 hours. It is expected to remain below the threshold during the next 24 hours. The 24h electron fluence was at normal level and is expected to remain so.
今日估計的國際太陽黑子數(ISN):093,基於07個觀測站。
| 卡塔尼亞沃爾夫數 | 108 |
| 10厘米太陽通量 | 127 |
| AK Chambon La Forêt | 009 |
| AK Wingst | 004 |
| 估計地磁Ap指數 | 004 |
| 估計國際太陽黑子數 | 074 - 基於14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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