發布時間: 2021 May 21 1231 UTC
Quiet conditions (<50% probability of C-class flares)
Quiet (A<20 and K<4)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 21 May 2021 | 072 | 013 |
| 22 May 2021 | 074 | 010 |
| 23 May 2021 | 076 | 007 |
Solar activity has been very low, only one active region visible: NOAA AR 2824 (Catania 96, alpha magnetic field configuration). Only B-class flares seen in 24 hours, some of them from a new active region rotating into view from the east limb, solar activity may increase as a result in the coming hours.
No Earth-directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraphic imagery in the last 24 hours.
The greater than 10 MeV proton flux was at nominal levels over the past 24 hours and is expected to remain so for the next 24 hours. The greater than 2 MeV electron flux remained below the 1000 pfu in the past 24 hours, it is expected to increase in the coming 24 hours. The 24-hour electron fluence was at normal levels in the past 24 hours, it is expected to increase in the coming 24 hours.
A high speed solar wind (HSS) stream arrived to the Earth in the past 24 hours. The speed increased to 600 km/s, with interplanetary magnetic field magnitudes up to 19 nT, with Bz reaching - 13 nT. The polarity of the magnetic field was mostly negative (towards the Sun). The solar wind speed is still elevated, but the magnetic field intensity has reduced to about 4 nT. Similar conditions are expected for the next 24 hours.
Geomagnetic conditions have reached minor storm levels (KDourbes 2-5, Kp 2-5) due to the HSS effect. Mostly unsettled conditions, with possible active periods, can be expected for the next 24 hours.
今日估計的國際太陽黑子數(ISN):013,基於19個觀測站。
| 卡塔尼亞沃爾夫數 | 026 |
| 10厘米太陽通量 | 072 |
| AK Chambon La Forêt | 035 |
| AK Wingst | 028 |
| 估計地磁Ap指數 | 027 |
| 估計國際太陽黑子數 | 018 - 基於32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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