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Solar Eclipses and the Surface Properties of Water
Earth, Moon, and Planets ( IF 0.9 ) Pub Date : 2019-09-30 , DOI: 10.1007/s11038-019-09529-0
Elmar C. Fuchs , Gerrit Oudakker , Martin Justinek , Nigel Dyer , Jakob Woisetschläger , Kevin Godines , Matthias Mäder , Friedemann T. Freund

During four solar eclipse events (two annular, one total and one partial) a correlation was observed between a change in water surface tension and the magnitude of the optical coverage. During one eclipse, evaporation experiments were carried out which showed a reduction in water evaporation at the same time as a rise in the surface tension. The changes did not occur on a day without a solar eclipse and are not correlated to changes in temperature, pressure, humidity of the environment. The effects are delayed by 20, 85, 30 and 37 min, respectively, compared to the maximum eclipse. Possible mechanisms responsible for this effect are presented, the most likely hypothesis being reduced water/muon interaction due to solar wind and cosmic radiation blocking during an eclipse. As an alternative hypotheses, we propose a novel neutrino/water interaction and overview of other, less likely mechanisms.

中文翻译:

日食和水的表面特性

在四次日食事件(两次环食、一次全食和一次部分日食)期间,观察到水表面张力的变化与光学覆盖范围的大小之间存在相关性。在一次日食期间,进行了蒸发实验,结果表明水蒸发减少,同时表面张力升高。这些变化不是在没有日食的一天发生的,并且与环境的温度、压力、湿度的变化无关。与最大日食相比,这些影响分别延迟了 20、85、30 和 37 分钟。介绍了造成这种效应的可能机制,最可能的假设是由于日食期间太阳风和宇宙辐射阻挡而减少了水/介子相互作用。作为替代假设,
更新日期:2019-09-30
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