Radio-Frequency Energy from the Sun
Radio-Frequency Energy from the Sun
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DOI：
10.1038/157158a0
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发表时间：
1946-02
期刊：
影响因子：
64.8
通讯作者：
J. Pawsey;R. PAYNE-SOOTT;L. McCready
中科院分区：
文献类型：
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作者：
J. Pawsey;R. PAYNE-SOOTT;L. McCready
Jansky1在1933年报告了似乎起源于银河系区域的10米波长范围内的射频辐射。他没有观察到来自太阳的可测量的影响，尽管它的热辐射远远超过了所有其他恒星的总辐射量，并推断这种“宇宙静态”起源于星际空间。后来的观察者，Reber2(2米)，英国陆军观察者3(5米)和新西兰皇家空军雷达人员(1.5米)，都报告了来自太阳本身的或小或大的影响。
RADIO-FREQUENCY radiation in the ten-metre range of wave-lengths which appeared to originate in the region of the Milky Way was reported by Jansky1in 1933. He observed no measurable effect from the sun, despite the fact that its thermal radiation immensely exceeds the total from all other stars, and deduced that this 'cosmic static' originated in interstellar space. Later observers, Reber2(2 metres), English Army observers3(5 metres) and Royal New Zealand Air Force radar personnel4(1.5 metres), have since reported small or large effects from the sun itself.