發布時間: 2026 Jan 12 1231 UTC
C-class flares expected, (probability >=50%)
Active conditions expected (A>=20 or K=4)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 12 Jan 2026 | 112 | 022 |
| 13 Jan 2026 | 114 | 031 |
| 14 Jan 2026 | 114 | 012 |
Solar flaring activity was moderate over the past 24 hours. The largest flare was a M3.3 flare (SIDC Flare 6631) peaking on January 11 at 23:14 UTC, originated from a region from behind the east limb. A total of 4 numbered sunspot groups are currently on the disk, all having alpha or beta magnetic configuration and have produced only C-class flaring. Solar flaring activity is expected to be low over the next 24 hours, with C-class flares very likely and a chance for M-class flares.
No new Earth-directed Coronal Mass Ejections (CMEs) have been detected in the available coronagraph images. The halo CME detected in SOHO/LASCO-C2 data from 23:36 UTC 11 JAN 2026, is backsided and not expected to arrive to the Earth.
Solar wind conditions were slightly elevated with speeds around 540 km/s. The interplanetary magnetic field was around 10nT, with the Bz reaching a minimum value of -10 nT. Solar wind conditions are expected to remain slightly elevated due to the ongoing ICME passage, and the possible arrival of high-speed streams from negative polarity coronal holes (SIDC Coronal Hole 137 and SIDC Coronal Hole 142).
Geomagnetic conditions reached minor storm levels globally and locally (Kp 5, K5) between 12:00 and 21:00 UTC on January 11 Mostly unsettled to active geomagnetic conditions are expected over the next day due to the ongoing ICME passage and possible HSS arrival.
The greater than 10 MeV proton flux remained below the 10 pfu threshold and is expected to remain so over the next days.
The greater than 2 MeV electron flux exceeded slightly the 1000 pfu threshold on 11 JAN between 21:35 UTC and 12 JAN 01:30 UTC and is currently slightly above the threshold since 10:45 UTC. The greater than 2 MeV electron flux is expected to have short crossings over the 1000 pfu threshold over the next 24 hours. The electron fluence was at normal levels and is expected to be at normal levels over the next 24 hours.
今日估計的國際太陽黑子數(ISN):049,基於08個觀測站。
| 卡塔尼亞沃爾夫數 | /// |
| 10厘米太陽通量 | 111 |
| AK Chambon La Forêt | 047 |
| AK Wingst | 032 |
| 估計地磁Ap指數 | 035 |
| 估計國際太陽黑子數 | 065 - 基於15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 |
|---|---|---|---|---|---|---|---|---|---|
| 11 | 2153 | 2314 | 0031 | ---- | M3.3 | --/---- |
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| 上一個 地球磁爆 | 16/05/2026 | Kp6- (G2) |
| 無黑子天數 | |
|---|---|
| 過去 365 天內 | 3天 |
| 2026 | 3天 (2%) |
| 上一個無黑子日 | 24/02/2026 |
| 黑子數月平均 | |
|---|---|
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