利用日偏食校准 14 米射电望远镜

IF 0.5 Q4 PHYSICS, APPLIED
J. Kallunki
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引用次数: 0

摘要

摘要 2022 年 10 月 25 日,欧洲中部和北部地区发生了日偏食。芬兰阿尔托大学 Metsähovi 射电天文台以 8 毫米 (37 千兆赫) 的射电波长观测到这次日偏食。芬兰境内的日偏食幅度为 62.7%。在整个日食过程中,以约 9 分钟的时间间隔观测到了太阳射电图。日食观测结果可用于仪器校准。本文利用上述日偏食观测数据研究太阳亮度温度、边缘增亮效应、色球高度和射电增亮位置。我们证实了先前的结果是一致的,例如太阳亮度温度与 8100 K ± 300 K 相吻合。不过,当时的太阳活动可能扭曲了最终结论。月球应该起到聚焦的作用,因此可以比正常情况下更仔细地确定射电增亮的位置。我们对这一特点进行了研究。我们的结果在某些方面出乎意料,需要进一步研究。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Using Partial Solar Eclipse for the 14-Metre Radio Telescope Calibration
Abstract A partial solar eclipse occurred on 25 October 2022, in the central and northern parts of Europe. The partial solar eclipse was observed at Aalto University Metsähovi Radio Observatory, Finland at the radio wavelength of 8 mm (37 GHz). In Finland, the magnitude of the partial solar eclipse was 62.7 %. Solar radio maps at the time cadence of about 9 minutes were observed over the whole eclipse. The solar eclipse observations could be used for instrument calibration purposes. This paper investigates the solar brightness temperature, the limb brightening effect, the height of the chromosphere and the location of radio brightening using the aforementioned partial solar eclipse observations. We got the confirmation that our earlier results are consistent, e.g., the solar brightness temperature matches with 8100 K ± 300 K. It was also possible to detect limb brightening effect. However, the prevailing solar activity might have distorted the final conclusions. The Moon should operate as a focusing element and the location of radio brightenings could be defined more carefully than in the normal conditions. We investigated this feature. Our results are in some parts unexpected and need further investigations.
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来源期刊
CiteScore
1.50
自引率
16.70%
发文量
41
审稿时长
5 weeks
期刊介绍: Latvian Journal of Physics and Technical Sciences (Latvijas Fizikas un Tehnisko Zinātņu Žurnāls) publishes experimental and theoretical papers containing results not published previously and review articles. Its scope includes Energy and Power, Energy Engineering, Energy Policy and Economics, Physical Sciences, Physics and Applied Physics in Engineering, Astronomy and Spectroscopy.
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