發布時間: 2023 Oct 07 1246 UTC
C-class flares expected, (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 07 Oct 2023 | 155 | 007 |
| 08 Oct 2023 | 155 | 007 |
| 09 Oct 2023 | 155 | 007 |
Solar flaring activity over the past 24 hours was quiet with only one small C-class flares beside the number of bipolar regions on the solar disc visible from Earth. There are currently 10 numbered active regions with alpha or beta magnetic field configurations. The most complex regions are NOAA AR 3451 (beta-gamma) and NOAA AR 3452 (beta-gamma). The solar flaring activity is likely to be at quiet levels over the coming days with C-class flares expected, and a low chance for isolated M-class flares and X-class flaring.
No other Earth-directed Coronal Mass Ejections have been detected in the last 24 hours in the available SOHO/LASCO images.
In the last 24 hours, the solar wind conditions near Earth remained slightly under the influence of the solar wind streams associated to 2 small positive polarity coronal holes that crossed the central meridian on October 01 and 02. The total interplanetary magnetic field was ranging between 5.0 nT and 7.3 nT. The Bz-component of the interplanetary magnetic showed mainly negative values with a minimum value of -4.6 nT. The solar wind speed had values varying between 337 km/s and 437 km/s. The solar wind is expected to return to nominal conditions in the next hours.
The geomagnetic conditions over the past 24 hours were quite to unsettled (K Bel 2-3, Kp-NOAA 2-3) due to the slight enhancement of the solar wind conditions. Quiet to unsettled conditions are expected in the next 24 hours.
The greater than 10 MeV proton flux was at background levels over the last 24 hours. It is expected to mostly remain at background level, however possible rise of the proton flux cannot be fully excluded due to the current number of complex regions on the disc.
The greater than 2 MeV electron flux measured by GOES-16 was below the 1000 pfu threshold. The greater than 2 MeV electron flux is expected remains below the threshold in the next 24 hours. The 24h electron fluence was at normal levels and is expected to remain at normal levels in the next 24 hours.
今日估計的國際太陽黑子數(ISN):126,基於15個觀測站。
| 卡塔尼亞沃爾夫數 | 193 |
| 10厘米太陽通量 | 155 |
| AK Chambon La Forêt | 012 |
| AK Wingst | 008 |
| 估計地磁Ap指數 | 007 |
| 估計國際太陽黑子數 | 152 - 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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