Helioseismic Constraints: Past, Current, and Future Observations

IF 2.7 3区物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS

Solar Physics Pub Date : 2024-11-13 DOI:10.1007/s11207-024-02403-x

Thierry Appourchaux

引用次数: 0

Abstract

I will review the history of the helioseismic observations since the beginning of the field. I will explain how each instrument was designed based upon the required observables, and to which modes these instruments are sensitive. The impact of these sensitivities on the rotation and structure inversion will be developed. I will conclude with what remains to be done in this field for the future of detection.

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太阳地震制约因素：过去、现在和未来的观测

我将回顾自该领域开始以来日震观测的历史。我将解释如何根据所需的观测数据设计每台仪器，以及这些仪器对哪些模式敏感。这些敏感性对自转和结构反演的影响将得到阐述。最后，我将介绍该领域在未来的探测方面还有哪些工作要做。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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来源期刊

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.