A multi-phase chronology of the Carrington storm of 1859 based on archival records of Trivandrum observatory

IF 2.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
R. Jayakrishnan, Fazil C K, Ajesh A
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Abstract

The rediscovery of bifilar magnetometer records from Trivandrum Observatory—preserved within the historical archives of the National Library of Scotland—provides a rare and independent equatorial dataset crucial for reassessing the intensity and temporal structure of the 1859 Carrington storm. These archival materials reveal a nuanced sequence of geomagnetic disturbances, in as response to a sequence of likely coronal mass ejection (CME) impacts on 16th August and 29th August preceding the well-known super storm of 2nd September, and subsequent magnetospheric disturbances on 5th, 13th and 15th September due to weaker CME events and/or solar wind streams. The analyses of the archived Aide’s bifilar magnetometer data show that the 29th August and 2nd September events were of comparable magnitude (\(\Delta \)H ≈ −1851 nT and \(\Delta \)H ≈ −1926 nT) respectively, positioning the former as a newly calibrated benchmark for pre-Carrington CME activity. The records evidence disrupted diurnal periodicity in the horizontal magnetic field intensity on 16th August, 5th September, 13th September and 15th September, underscoring the magnetospheric fluctuations which may have been induced by successive interplanetary CME (ICME) impacts. By leveraging these meticulously preserved observatory logs, this study reconstructs a multi-phase chronology of the Carrington storm.

基于特里凡得琅天文台档案记录的1859年卡林顿风暴的多阶段年表
特里凡得勒姆天文台双线磁力计记录的重新发现——保存在苏格兰国家图书馆的历史档案中——为重新评估1859年卡灵顿风暴的强度和时间结构提供了一个罕见的、独立的赤道数据集。这些档案资料揭示了一系列细微的地磁扰动,作为对8月16日和8月29日一系列可能的日冕物质抛射(CME)影响的响应,在9月2日众所周知的超级风暴之前,以及随后9月5日,13日和15日由于较弱的CME事件和/或太阳风流造成的磁层扰动。对已存档的Aide双线磁力计数据的分析表明,8月29日和9月2日的事件分别具有相当的震级(\(\Delta \) H≈−1851 nT和\(\Delta \) H≈−1926 nT),将前者定位为卡灵顿前CME活动的新校准基准。这些记录表明,8月16日、9月5日、9月13日和9月15日水平磁场强度的日周期性被打乱,强调了磁层波动可能是由连续的行星际CME (ICME)撞击引起的。通过利用这些精心保存的观测日志,本研究重建了卡灵顿风暴的多阶段年表。
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来源期刊
Astrophysics and Space Science
Astrophysics and Space Science 地学天文-天文与天体物理
CiteScore
3.40
自引率
5.30%
发文量
106
审稿时长
2-4 weeks
期刊介绍: Astrophysics and Space Science publishes original contributions and invited reviews covering the entire range of astronomy, astrophysics, astrophysical cosmology, planetary and space science and the astrophysical aspects of astrobiology. This includes both observational and theoretical research, the techniques of astronomical instrumentation and data analysis and astronomical space instrumentation. We particularly welcome papers in the general fields of high-energy astrophysics, astrophysical and astrochemical studies of the interstellar medium including star formation, planetary astrophysics, the formation and evolution of galaxies and the evolution of large scale structure in the Universe. Papers in mathematical physics or in general relativity which do not establish clear astrophysical applications will no longer be considered. The journal also publishes topically selected special issues in research fields of particular scientific interest. These consist of both invited reviews and original research papers. Conference proceedings will not be considered. All papers published in the journal are subject to thorough and strict peer-reviewing. Astrophysics and Space Science features short publication times after acceptance and colour printing free of charge.
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