發布時間: 2024 May 23 1231 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 | |
|---|---|---|
| 23 May 2024 | 196 | 007 |
| 24 May 2024 | 194 | 011 |
| 25 May 2024 | 192 | 010 |
There are six visible ARs on the solar disk. There were four M-class flares in the last 24 hours, from NOAA 3679 (that evolved into beta-gamma-delta magnetic field configuration). The strongest one was an M4.2 peaking at 02:16 UTC. NOAA AR 3683 rotated over the west limb, but is still producing significant flares (C9.8 at 07:01 UTC). NOAA AR 3685 (beta gamma magnetic field configuration) has also potential for strong flaring activity. For the next 24 hours, more M-class flares can be expected and X-class flares are possible.
No Earth directed CME has been observed in the last 24 hours.
A negative polarity coronal hole in the northern hemisphere has developed a low latitudinal extension that traversed the central meridian on 21 May. A possible arrival of high speed steam from this coronal hole could arrive at the Earth (late) on 24 May.
The solar wind at the Earth is slow, with speeds around 400 km/s and interplanetary magnetic field around 7 nT. Similar conditions can be expected for the next 24 hours.
Geomagnetic conditions have been quiet in the last 24 hours (Kp and K_BEL up to 2). Similar quiet conditions can be expected for the next 24 hours.
The 10 MeV GOES-18 proton flux was below threshold in the past 24 hours. Since some of the regions producing the M-class flaring are close to the west limb, a proton event cannot be discarded in the next 24 hours.
The greater than 2 MeV electron flux from GOES 16 was below the threshold level in the last 24 hours. It is expected to remain below the threshold during the next 24 hours. The electron fluence was at normal levels for the last 24 hours and is expected to remain so.
今日估計的國際太陽黑子數(ISN):135,基於15個觀測站。
| 卡塔尼亞沃爾夫數 | 188 |
| 10厘米太陽通量 | 196 |
| AK Chambon La Forêt | 008 |
| AK Wingst | 005 |
| 估計地磁Ap指數 | 004 |
| 估計國際太陽黑子數 | 151 - 基於21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 |
|---|---|---|---|---|---|---|---|---|---|
| 22 | 1351 | 1405 | 1412 | S06W55 | M1.2 | SF | 06/3679 | ||
| 23 | 0205 | 0216 | 0226 | ---- | M4.2 | 06/3679 | |||
| 23 | 0403 | 0429 | 0454 | S09W18 | M1.7 | SF | 06/3679 | VI/2 |
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