Clouds and the Near-Earth Environment: Possible Links

S. Condurache-Bota, M. Voiculescu, C. Dragomir
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Abstract

Abstract Climate variability is a hot topic not only for scientists and policy-makers, but also for each and every one of us. The anthropogenic activities are considered to be responsible for most climate change, however there are large uncertainties about the magnitude of effects of solar variability and other extraterrestrial influences, such as galactic cosmic rays on terrestrial climate. Clouds play an important role due to feedbacks of the radiation budget: variation of cloud cover/composition affects climate, which, in turn, affects cloud cover via atmospheric dynamics and sea temperature variations. Cloud formation and evolution are still under scientific scrutiny, since their microphysics is still not understood. Besides atmospheric dynamics and other internal climatic parameters, extraterrestrial sources of cloud cover variation are considered. One of these is the solar wind, whose effect on cloud cover might be modulated by the global atmospheric electrical circuit. Clouds height and composition, their seasonal variation and latitudinal distribution should be considered when trying to identify possible mechanisms by which solar energy is transferred to clouds. The influence of the solar wind on cloud formation can be assessed also through the ap index - the geomagnetic storm index, which can be readily connected with interplanetary magnetic field, IMF structure. This paper proposes to assess the possible relationship between both cloud cover and solar wind proxies, as the ap index, function of cloud height and composition and also through seasonal studies. The data covers almost three solar cycles (1984-2009). Mechanisms are looked for by investigating observed trends or correlation at local/seasonal scale
云和近地环境:可能的联系
气候变率不仅是科学家和决策者的热门话题,也是我们每一个人的热门话题。人类活动被认为是造成大多数气候变化的原因,然而,太阳变率和其他地外影响,如银河宇宙射线对地球气候的影响程度存在很大的不确定性。由于辐射收支的反馈,云起着重要的作用:云量/组成的变化影响气候,而气候又通过大气动力学和海温变化影响云量。云的形成和演化仍然在科学的审视之下,因为它们的微观物理学仍然没有被理解。除了大气动力学和其他内部气候参数外,还考虑了云量变化的地外来源。其中之一是太阳风,它对云层覆盖的影响可能会被全球大气电路调制。在试图确定太阳能向云转移的可能机制时,应考虑云的高度和组成、季节变化和纬度分布。太阳风对云形成的影响也可以通过地磁风暴指数来评估,地磁风暴指数可以很容易地与行星际磁场、IMF结构联系起来。本文建议通过ap指数、云高和组成的函数以及季节研究来评估云量和太阳风指标之间可能存在的关系。这些数据涵盖了几乎三个太阳活动周期(1984-2009)。通过调查在当地/季节尺度上观察到的趋势或相关性来寻找机制
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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