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On the relation between rain, clouds, and cosmic rays

宇宙射线 临近预报 宇宙癌症数据库 环境科学 太阳黑子 物理 降水 气象学 天体物理学 磁场 量子力学
作者
C. Varotsos,Г. С. Голицын,Yong Xue,M. Efstathiou,N. V. Sarlis,Tatiana Voronova
出处
期刊:Remote Sensing Letters [Taylor & Francis]
卷期号:14 (3): 301-312 被引量:12
标识
DOI:10.1080/2150704x.2023.2190468
摘要

ABSTRACTWe investigate the correlation between precipitation, clouds and cosmic rays based on field observations to develop a new short-term forecasting tool for their extremely high values. The results show that the cosmic ray intensity appears to be highly correlated with the one-year time-lagged rainfall amount with the cosmic rays leading. A plausible explanation is given for this, based on the modulation of cosmic rays by the solar cycle and an earlier finding of a strong correlation between the stratospheric - lower mesospheric temperature fluctuations and the sunspot number cycle with a time lag of one year (sun leading). This suggests that cosmic rays are not the trigger, but rather signals sunspot activity that with a delay of one year may affect cloud formation and therefore rainfall. In addition, high rates of rainfall exhibit a power-law behavior, such as the Gutenberg-Richter law characterizing the large area and perimeter size of rainfall and clouds, which have been proposed recently. Finally, the new tool for the nowcasting the extremely high cosmic ray intensity values can be used for nowcasting the extremely high rainfall values. Their combination can be used to study the modulation of cosmic ray properties by climate change parameters.KEYWORDS: extreme eventsraincloudscosmic rayssolar cyclenowcasting AcknowledgmentsThis research was carried out in the framework of the Program Agreement between 'Ministry of Digital Governance' (Greece) and the 'National & Kapodistrian University of Athens Greece (Research Code: 18434). We acknowledge the NMDB database www.nmdb.eu, founded under the European Union's FP7 programme (contract no. 213007) for providing data. Athens neutrons monitor data were kindly provided by the Physics Faculty of the National and Kapodistrian University of Athens.Disclosure statementNo potential conflict of interest was reported by the authors.Additional informationFundingThe work was supported by the 'Ministry of Digital Governance (Greece) [Research Code: 18434].
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