Earth's Mesosphere During Possible Encounters With Massive Interstellar Clouds 2 and 7 Million Years Ago

Jesse A. Miller, Merav Opher, Maria Hatzaki, Kyriakoula Papachristopoulou, Brian C. Thomas
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Abstract

Our solar system's path has recently been shown to potentially intersect dense interstellar clouds 2 and 7 million years ago: the Local Lynx of Cold Cloud and the edge of the Local Bubble. These clouds compressed the heliosphere, directly exposing Earth to the interstellar medium. Previous studies that examined climate effects of these encounters argued for an induced ice age due to the formation of global noctilucent clouds (NLCs). Here, we revisit such studies with a modern 2D atmospheric chemistry model using parameters of global heliospheric magnetohydrodynamic models as input. We show that NLCs remain confined to polar latitudes and short seasonal lifetimes during these dense cloud crossings lasting $\sim10^5$ years. Polar mesospheric ozone becomes significantly depleted, but the total ozone column broadly increases. Furthermore, we show that the densest NLCs lessen the amount of sunlight reaching the surface instantaneously by up to 7% while halving outgoing longwave radiation.
200 万年前和 700 万年前可能遭遇大规模星际云时的地球中间层
最近的研究表明,我们太阳系的运行轨迹有可能在200万年前和700万年前与密集的星际云相交:冷云的地方山猫和地方气泡的边缘。这些云压缩了日光层,使地球直接暴露在星际介质中。以前的研究考察了这些遭遇对气候的影响,认为全球夜光云(NLCs)的形成诱发了冰期。在这里,我们使用现代二维大气化学模型,以全球日光层磁流体动力学模型参数为输入,对这些研究进行了考察。我们的研究表明,NLCs仍然局限于极地纬度,并且在这些浓云穿越期间的季节寿命很短,持续时间为10^5年。极地中层臭氧会明显耗竭,但总臭氧柱会广泛增加。此外,我们还表明,密度最大的 NLCs 会将瞬间到达地表的太阳光量减少高达 7%,同时将流出的长波辐射减半。
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