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The Greenwich Photo-heliographic Results (1874 - 1976): Summary of the Observations, Applications, Datasets, Definitions and Errors

机译:格林威治光合照相结果(1874年至1976年):观测,应用,数据集,定义和错误的摘要

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摘要

The measurements of sunspot positions and areas that were published initially by the Royal Observatory, Greenwich, and subsequently by the Royal Greenwich Observatory (RGO), as the Greenwich Photo-heliographic Results (GPR), 1874 - 1976, exist in both printed and digital forms. These printed and digital sunspot datasets have been archived in various libraries and data centres. Unfortunately, however, typographic, systematic and isolated errors can be found in the various datasets. The purpose of the present paper is to begin the task of identifying and correcting these errors. In particular, the intention is to provide in one foundational paper all the necessary background information on the original solar observations, their various applications in scientific research, the format of the different digital datasets, the necessary definitions of the quantities measured, and the initial identification of errors in both the printed publications and the digital datasets. Two companion papers address the question of specific identifiable errors; namely, typographic errors in the printed publications, and both isolated and systematic errors in the digital datasets. The existence of two independently prepared digital datasets, which both contain information on sunspot positions and areas, makes it possible to outline a preliminary strategy for the development of an even more accurate digital dataset. Further work is in progress to generate an extremely reliable sunspot digital dataset, based on the programme of solar observations supported for more than a century by the Royal Observatory, Greenwich, and the Royal Greenwich Observatory. This improved dataset should be of value in many future scientific investigations.
机译:太阳黑子位置和面积的测量最初由格林威治皇家天文台发布,随后由皇家格林威治天文台(RGO)发布,作为1874年至1976年的格林威治照片平版印刷结果(GPR),目前以印刷形式和数字形式存在形式。这些印刷的和数字黑子数据集已在各个图书馆和数据中心存档。但是,不幸的是,可以在各种数据集中找到印刷错误,系统错误和孤立错误。本文的目的是开始识别和纠正这些错误的任务。尤其是,其目的是在一份基础论文中提供有关原始太阳观测,其在科学研究中的各种应用,不同数字数据集的格式,所测量数量的必要定义以及初始识别的所有必要背景信息。印刷出版物和数字数据集中的错误。有两篇配套文件讨论了具体可识别错误的问题;即印刷出版物中的印刷错误,以及数字数据集中的孤立性和系统性错误。存在两个独立准备的数字数据集,这两个数据集都包含有关黑子位置和面积的信息,因此可以勾勒出开发更准确的数字数据集的初步策略。根据皇家天文台,格林威治和皇家格林威治天文台支持一个多世纪的太阳观测计划,正在进行进一步工作以生成极其可靠的太阳黑子数字数据集。改进后的数据集应在未来的许多科学研究中具有价值。

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