{"title":"130 years of spectroheliograms at Paris-Meudon observatories (1893–2023)","authors":"J. Malherbe","doi":"10.1177/00218286231184193","DOIUrl":null,"url":null,"abstract":"Broad-band observations of the solar photosphere began in Meudon in 1875 under the auspices of Jules Janssen. For his part, Henri Deslandres initiated imaging spectroscopy in 1892 at Paris observatory. He invented, concurrently with George Hale in Kenwood (USA), but quite independently, the spectroheliograph designed for monochromatic imagery of the solar atmosphere. Deslandres developed two kinds of spectrographs: the ‘spectrohéliographe des formes’, that is, the narrow bandpass instrument to reveal chromospheric structures; and the ‘spectrohéliographe des vitesses’, that is, the section spectroheliograph to record line profiles of cross sections of the Sun. This second apparatus was intended to measure the Dopplershifts of dynamic features. Deslandres moved to Meudon in 1898 to build the large quadruple spectroheliograph. The service of Hα and CaII K systematic observations was organized by Lucien d’Azambuja and continues today. The digital technology was introduced in 2002. The collection is one of the longest available: it contains sporadic images from 1893 to 1907 (during the development phase) and systematic observations along 10 solar cycles since 1908. This paper summarizes 130 years of observations, instrumental research and technical advances.","PeriodicalId":56280,"journal":{"name":"Journal for the History of Astronomy","volume":"54 1","pages":"274 - 315"},"PeriodicalIF":0.3000,"publicationDate":"2023-08-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal for the History of Astronomy","FirstCategoryId":"98","ListUrlMain":"https://doi.org/10.1177/00218286231184193","RegionNum":3,"RegionCategory":"哲学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"HISTORY & PHILOSOPHY OF SCIENCE","Score":null,"Total":0}
引用次数: 0
Abstract
Broad-band observations of the solar photosphere began in Meudon in 1875 under the auspices of Jules Janssen. For his part, Henri Deslandres initiated imaging spectroscopy in 1892 at Paris observatory. He invented, concurrently with George Hale in Kenwood (USA), but quite independently, the spectroheliograph designed for monochromatic imagery of the solar atmosphere. Deslandres developed two kinds of spectrographs: the ‘spectrohéliographe des formes’, that is, the narrow bandpass instrument to reveal chromospheric structures; and the ‘spectrohéliographe des vitesses’, that is, the section spectroheliograph to record line profiles of cross sections of the Sun. This second apparatus was intended to measure the Dopplershifts of dynamic features. Deslandres moved to Meudon in 1898 to build the large quadruple spectroheliograph. The service of Hα and CaII K systematic observations was organized by Lucien d’Azambuja and continues today. The digital technology was introduced in 2002. The collection is one of the longest available: it contains sporadic images from 1893 to 1907 (during the development phase) and systematic observations along 10 solar cycles since 1908. This paper summarizes 130 years of observations, instrumental research and technical advances.
1875年,在朱尔斯·杨森的主持下,在默顿开始了对太阳光球层的宽带观测。亨利·德斯兰德雷斯于1892年在巴黎天文台开创了成像光谱学。他与乔治·黑尔(George Hale)在肯伍德(美国)同时但相当独立地发明了为太阳大气的单色图像设计的分光光度计。Deslandres开发了两种光谱仪:“spectrohéliographe des formes”,即显示色球结构的窄带仪器;以及“viteshéliographe des vitesses”,即记录太阳横截面线形的截面分光镜。第二个装置旨在测量动态特征的Dopplershift。1898年,Deslandres搬到了Meudon,建造了大型的四重日谱仪。Hα和CaII K系统观测服务由Lucien d’Azambuja组织,至今仍在继续。数字技术于2002年引入。该藏品是可用时间最长的藏品之一:它包含1893年至1907年(在开发阶段)的零星图像和1908年以来10个太阳周期的系统观测。本文总结了130 多年的观测、仪器研究和技术进步。
期刊介绍:
Science History Publications Ltd is an academic publishing company established in 1971 and based in Cambridge, England. We specialize in journals in history of science and in particular history of astronomy.