查看星期二, 31 3月 2015歷史檔案

SIDC 太陽影響數據分析中心的每日公告

發布時間: 2015 Mar 31 1230 UTC

SIDC太陽影響數據分析中心的預報

從 1230 UTC, 31 Mar 2015 到 02 Apr 2015 都有效
太陽閃焰

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

地磁

Minor storm expected (A>=30 or K=5)

太陽質子

Quiet

10公分通量Ap
31 Mar 2015132017
01 Apr 2015128020
02 Apr 2015125008

公告

Flaring activity during the last 24 hours was limited to four C-class flares. The strongest flare was a C4.1 flare peaking at 22:05 UT on March 30 originating from the NOAA active region (AR) 2303, located right behind the west limb. We expect flaring activity at the low C-level in the next 48 hours, potentially from NOAA ARs 2315 and 2316. No Earth-directed CMEs were observed. The Earth is still inside a slow solar wind flow. A shock-like signature was observed in the solar wind data observed by ACE and SOHO/CELIAS. Solar wind speed (to about 400 km/s), density and the magnitude of the interplanetary magnetic field (IMF) jumped at around 7:40 UT on March 31. The z-component of the IMF is varying between -13 and +11 nT. The solar source of this disturbance in the solar wind is unclear at this moment. A CME from March 27 (first measurement in LASCO-C2 at 13:36 UT) and a CME of March 28 (fist detected in LASCO-C2 around 10:37 UT) are two potentially associated events. No geomagnetic disturbances are noted yet. Geomagnetic activity up to the minor storm level is expected, due to the combined influence of the arrived shock-like structure and the fast flow from a low-latitude extension of the southern polar coronal hole, which is expected to arrive in the course of today.

今日估計的國際太陽黑子數(ISN):031,基於15個觀測站。

太陽活動指數 30 Mar 2015

卡塔尼亞沃爾夫數060
10厘米太陽通量134
AK Chambon La Forêt006
AK Wingst006
估計地磁Ap指數005
估計國際太陽黑子數042 - 基於27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

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