毫米射电天文学作为对太阳对流区的探测

2010 INTERNATIONAL KHARKOV SYMPOSIUM ON PHYSICS AND ENGINEERING OF MICROWAVES, MILLIMETER AND SUBMILLIMETER WAVES Pub Date : 2010-06-21 DOI:10.1109/MSMW.2010.5546109

O. V. Arkhypov, A. Antonov

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引用次数: 0

摘要

较小的毫米射电望远镜相对较低的空间分辨率缩小了太阳物理领域可用任务的范围。然而，太阳上的大规模现象隐藏在雇佣图像的细节之中。例如，太阳活动的全球分布显然与对流区深处的过程有关。

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Millimeter radio astronomy as a probe for convective zone of the Sun

Relatively low spatial resolution of not great millimeter radio-telescopes narrows the range of available tasks in the field of solar physics. However, there are large scale phenomena on the Sun hidden among fine details of hires images. For example, the global distribution of solar activity is apparently connected with the processes in the depths of the convection zone.

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来源期刊

2010 INTERNATIONAL KHARKOV SYMPOSIUM ON PHYSICS AND ENGINEERING OF MICROWAVES, MILLIMETER AND SUBMILLIMETER WAVES

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