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Midlatitude cooling caused by geomagnetic field minimum during polarity reversal

机译:极性反转期间最小的地磁场引起的中纬度冷却

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摘要

The climatic effects of cloud formation induced by galactic cosmic rays (CRs) has recently become a topic of much discussion. The CR–cloud connection suggests that variations in geomagnetic field intensity could change climate through modulation of CR flux. This hypothesis, however, is not well-tested using robust geological evidence. Here we present paleoclimate and paleoenvironment records of five interglacial periods that include two geomagnetic polarity reversals. Marine oxygen isotope stages 19 and 31 contain both anomalous cooling intervals during the sea-level highstands and the Matuyama–Brunhes and Lower Jaramillo reversals, respectively. This contrasts strongly with the typical interglacial climate that has the temperature maximum at the sea-level peak. The cooling occurred when the field intensity dropped to <40% of its present value, for which we estimate >40% increase in CR flux. The climate warmed rapidly when field intensity recovered. We suggest that geomagnetic field intensity can influence global climate through the modulation of CR flux.
机译:银河系宇宙射线(CR)引起的云形成的气候效应最近已成为许多讨论的话题。 CR-云的关系表明,地磁场强度的变化可能通过调节CR通量来改变气候。但是,该假设尚未使用可靠的地质证据进行充分检验。在这里,我们介绍了五个间冰期的古气候和古环境记录,其中包括两次地磁极性反转。海洋氧同位素第19级和第31级分别包含在海平面高位以及Matuyama-Brunhes和Lower Jaramillo逆转期间的异常冷却间隔。这与典型的间冰期气候形成鲜明对比,后者在海平面峰值处具有最高温度。当场强降至其当前值的<40%时发生冷却,为此我们估计CR通量增加> 40%。当场强恢复时,气候迅速变暖。我们建议地磁场强度可以通过调节CR通量来影响全球气候。

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