红外太阳物理学

IF 20.9 1区物理与天体物理

Living Reviews in Solar Physics Pub Date : 2014-03-21 DOI:10.12942/lrsp-2014-2

Matthew J. Penn

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引用次数: 55

摘要

太阳红外光谱包含了大量关于太阳的物理数据，并使用现代探测器和技术与新的地面太阳望远镜进行了探索。本文介绍了探索这些波长背后的科学动机，并简要介绍了这里丰富的观测历史。讨论了利用1000 ~ 12 400 nm红外波段观测的几种太阳物理研究途径，并简要总结了推动这一研究的仪器和探测器技术。最后，结合地面和天基观测，提出了未来红外波长工作的目标。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

Infrared Solar Physics

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Infrared Solar Physics

The infrared solar spectrum contains a wealth of physical data about our Sun, and is explored using modern detectors and technology with new ground-based solar telescopes. The scientific motivation behind exploring these wavelengths is presented, along with a brief look at the rich history of observations here. Several avenues of solar physics research exploiting and benefiting from observations at infrared wavelengths from roughly 1000 nm to 12 400 nm are discussed, and the instrument and detector technology driving this research is briefly summarized. Finally, goals for future work at infrared wavelengths are presented in conjunction with ground and space-based observations.

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来源期刊

Living Reviews in Solar Physics ASTRONOMY & ASTROPHYSICS-

自引率

1.40%

发文量

期刊介绍： Living Reviews in Solar Physics, a platinum open-access journal, publishes invited reviews covering research across all areas of solar and heliospheric physics. It distinguishes itself by maintaining a collection of high-quality reviews regularly updated by the authors. Established in 2004, it was founded by the Max Planck Institute for Solar System Research (MPS). "Living Reviews®" is a registered trademark of Springer International Publishing AG.