發布時間: 2025 Mar 05 1231 UTC
M-class flares expected (probability >=50%)
Quiet (A<20 and K<4)
Quiet
| 10公分通量 | Ap | |
|---|---|---|
| 05 Mar 2025 | 161 | 008 |
| 06 Mar 2025 | 155 | 006 |
| 07 Mar 2025 | 150 | 005 |
Solar flaring activity was moderate over the past 24 hours, with an M1.7 flare emitted from SIDC Sunspot Group 423 (NOAA Active Region 4012, at S13E28, Beta-Gamma magnetic configuration) 5 Mar at 11:50 UTC. During the next 24 hours further M-class flaring from the same SIDC sunspot group is likely to take place.
No Earth-directed Coronal Mass Ejections (CME) were observed in the last 24 hours.
The Solar Wind (SW) conditions were affected by a minor glancing blow from a Coronal Mass Ejection (CME) launched on 1 Mar, that arrived a few hours earlier than expected. However, this event had a minor effect on the SW conditions that were mostly typical of the slow regime. The SW speed gradually decreased from 530 to 410 km/s, while the interplanetary magnetic field (B) ranged between 3 to 9 nT in the last 24 hours. Its North-South component (Bz) registered values between -8 and 7 nT during the same period. The SW conditions are expected to remain in the slow SW regime over the next 24 hours.
The geomagnetic conditions gradually reached active levels both globally and locally (NOAA Kp 4+ and K BEL 4) between 4 Mar 21:00 and 24:00 UTC. However, after 5 Mar 03:00 UTC the conditions dropped back to quiet levels and they are expected to raise up to unsettled levels both globally and locally in the next 24 hours.
The greater than 10 MeV proton flux, as measured by the GOES-18 satellite, was at nominal levels over the past 24 hours and is likely to remain so in the next 24 hours.
The greater than 2 MeV electron flux, as measured by the GOES-18 satellite, marginally exceed the 1000 pfu threshold on 4 Mar between 18:05 and 23:45 UTC. For the next 24 hours it is expected to remain at this level. The 24h electron fluence decreased to normal levels over the past 24 hours. It is expected to remain at normal levels, but stay close to the moderate threshold during the next 24 hours.
今日估計的國際太陽黑子數(ISN):148,基於19個觀測站。
| 卡塔尼亞沃爾夫數 | 189 |
| 10厘米太陽通量 | 160 |
| AK Chambon La Forêt | 026 |
| AK Wingst | 013 |
| 估計地磁Ap指數 | 014 |
| 估計國際太陽黑子數 | 159 - 基於25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 |
|---|---|---|---|---|---|---|---|---|---|
| 05 | 1145 | 1150 | 1154 | ---- | M1.7 | --/---- | III/1 |
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| 上一個 M-閃焰 | 20/12/2025 | M1.0 |
| 上一個 地球磁爆 | 12/12/2025 | Kp5 (G1) |
| 無黑子天數 | |
|---|---|
| 上一個無黑子日 | 08/06/2022 |
| 黑子數月平均 | |
|---|---|
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