From the Wolf number to the International Sunspot Index: 25 years of SIDC

被引:112
作者
Clette, Frederic [1 ]
Berghmans, David [1 ]
Vanlommel, Petra [1 ]
Van der Linden, Ronald A. M. [1 ]
Koeckelenbergh, Andre [1 ]
Wauters, Laurence [1 ]
机构
[1] Royal Observ Belgium, Solar Influences Data Anal Ctr, B-1180 Brussels, Belgium
关键词
solar activity; sunspots; activity indices; photosphere; observing techniques;
D O I
10.1016/j.asr.2006.12.045
中图分类号
V [航空、航天];
学科分类号
08 [工学]; 0825 [航空宇航科学与技术];
摘要
By encompassing four centuries of solar evolution, the sunspot number provides the longest available record of solar activity. Nowadays, it is widely used as the main reference solar index on which hundreds of published studies are based, in various fields of science. In this review, we will retrace the history of this crucial solar index, from its roots at the Zurich Observatory up to the current multiple indices established and distributed by the Solar Influences Data Analysis Center (SIDC), World Data Center for the International Sunspot Index, which was founded in 1981, exactly 25 years ago. We describe the principles now in use for the statistical processing of input data coming from the worldwide observing network (similar to 80 stations). Among the various SIDC data products and innovations, we highlight some recent ones, including the daily Estimated International Sunspot Number. Taking a wider perspective, we show how the sunspot index stands the test of time versus more recent quantitative indices, but we also consider the prospects and possible options for a future transition from the visual sunspot index heritage towards an equivalent global activity index. Based on past historical flaws, we conclude on the key requirements involved in the maintenance of any robust long-term solar activity index. (C) 2007 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:919 / 928
页数:10
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