查看星期五, 2 5月 2014歷史檔案

SIDC 太陽影響數據分析中心的每日公告

發布時間: 2014 May 02 1335 UTC

SIDC太陽影響數據分析中心的預報

從 1230 UTC, 02 May 2014 到 04 May 2014 都有效
太陽閃焰

Eruptive (C-class flares expected, probability >=50%)

地磁

Quiet (A<20 and K<4)

太陽質子

Quiet

10公分通量Ap
02 May 2014135011
03 May 2014140003
04 May 2014140006

公告

Flaring activity has slightly increased during the past 24 hours. Two C-class flares were produced by Catania sunspot group 33 (NOAA AR 2047). The C4.4 flare, peaking at 9:40 UT, on 2 May was accompanied by a coronal dimming located at the south of the region. This hints at the occurrence of CME oriented to the south, but no coronagraphic imagery is available yet to analysis this. Catania sunspot groups 33 and 34 (NOAA AR 2047 and 2049 resp) showed some growth and sunspot group 33 now also has a beta-gamma magnetic configuration of its photospheric field. Two new sunspot groups emerged with Catania numbers 36 and 37. More C-class flares can be expected, especially from sunspot groups 33 and 34. There is moderate chance (around 40%) for M-class flares. We are currently under the influence of a slow solar wind. The solar wind speed decreased 400 to 340 km/s. The magnitude of the interplanetary magnetic field went from 8 to 2 nT. Geomagnetic conditions were quiet to unsettled and are expected to remain as such for the next 48 hours. The slow CME of UT night of 29-30 April could arrive at around 5 May 0:00 UT, possibly leading to a limited time of active conditions.

今日估計的國際太陽黑子數(ISN):081,基於13個觀測站。

太陽活動指數 01 May 2014

卡塔尼亞沃爾夫數///
10厘米太陽通量126
AK Chambon La Forêt008
AK Wingst005
估計地磁Ap指數005
估計國際太陽黑子數064 - 基於22個觀測站

顯著活動摘要

開始最大值結束位置強度OP10cm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

由太陽影響數據分析中心提供© - SIDC - 由 SpaceWeatherLive處理

所有時間均採用 UTC 時間

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