IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Nadezhda Zolotova, Mikhail Vokhmyanin
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引用次数: 0

摘要

我们分析了 1660 - 1676 年间的太阳黑子雕刻和测量数据,以获取太阳黑子面积和太阳坐标。根据这些数据,我们修正了霍伊特和沙滕(《太阳在气候变化中的作用》,1997 年)关于在莫德极小期出现长寿命太阳黑子是对流减弱迹象的假设。历史报告还澄清了每位观测者对太阳黑子的定义以及观测的目的。通过重建的太阳黑子经度,我们可以评估旋转率,发现历史上的旋转轮廓与现代长寿命太阳黑子群的旋转轮廓相似。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Long-Lived Sunspots in Historical Records: A Case Study Analysis from 1660 to 1676

We analyze Sunspot engravings and measurements in 1660 – 1676 to retrieve sunspot area and heliocoordinates. Based on these data, we revise the Hoyt and Schatten (The role of the sun in climate change, 1997) hypothesis of long-lived sunspots during the Maunder minimum as a sign of weakened convection. Historical reports also clarify what each observer defined as a sunspot and the purpose of the observations. The reconstructed longitudes of sunspots allow us to evaluate the rotation rate, revealing that the historical rotation profile resembles that of long-lived sunspot groups in the modern era.

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来源期刊
Solar Physics
Solar Physics 地学天文-天文与天体物理
CiteScore
5.10
自引率
17.90%
发文量
146
审稿时长
1 months
期刊介绍: Solar Physics was founded in 1967 and is the principal journal for the publication of the results of fundamental research on the Sun. The journal treats all aspects of solar physics, ranging from the internal structure of the Sun and its evolution to the outer corona and solar wind in interplanetary space. Papers on solar-terrestrial physics and on stellar research are also published when their results have a direct bearing on our understanding of the Sun.
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