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The Greenwich Photo-heliographic Results (1874 – 1976): Initial Corrections to the Printed Publications

机译:格林威治照相平版印刷的结果(1874年至1976年):印刷出版物的初步更正

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A new sunspot and faculae digital dataset for the interval 1874 – 1955 has been prepared under the auspices of the NOAA National Geophysical Data Center (NGDC). This digital dataset contains measurements of the positions and areas of both sunspots and faculae published initially by the Royal Observatory, Greenwich, and subsequently by the Royal Greenwich Observatory (RGO), under the title Greenwich Photo-heliographic Results (GPR), 1874 – 1976. Quality control (QC) procedures based on logical consistency have been used to identify the more obvious errors in the RGO publications. Typical examples of identifiable errors are North versus South errors in specifying heliographic latitude, errors in specifying heliographic (Carrington) longitude, errors in the dates and times, errors in sunspot group numbers, arithmetic errors in the summation process, and the occasional omission of solar ephemerides. Although the number of errors in the RGO publications is remarkably small, an initial table of necessary corrections is provided for the interval 1874 – 1917. Moreover, as noted in the preceding companion papers, 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 long programme of solar observations supported first by the Royal Observatory, Greenwich, and then by the Royal Greenwich Observatory.
机译:在NOAA国家地球物理数据中心(NGDC)的主持下,准备了一个新的太阳黑子和小分子数字数据集,其范围为1874 -1955年。该数字数据集包含最初由格林威治天文台,随后由皇家格林威治天文台(RGO)发布,标题为“格林威治照相平版印刷结果(GPR),1874年-1976年”的太阳黑子和微透镜的位置和面积的测量值基于逻辑一致性的质量控制(QC)程序已用于识别RGO出版物中更明显的错误。可识别的错误的典型示例是指定纬度的南北误差,指定纬度(卡灵顿)的误差,日期和时间的误差,黑子群编号的误差,求和过程中的算术误差以及偶尔遗漏太阳星历表。尽管RGO出版物中的错误数量非常少,但是为1874 -1917年间的间隔提供了必要的更正的初始表格。此外,如前面的伴随文件所述,存在两个独立准备的数字数据集,它们都包含有关太阳黑子位置和区域的信息,可以勾勒出发展更准确的数字数据集的初步策略。根据长期的太阳观测计划,进一步的工作正在生成一个极其可靠的黑子数字数据集,该计划首先由格林威治皇家天文台支持,然后由皇家格林威治天文台支持。

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