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观测到蓝色喷流进入平流层。

Observation of the onset of a blue jet into the stratosphere.

机构信息

National Space Institute, Technical University of Denmark (DTU Space), Kongens Lyngby, Denmark.

Birkeland Centre for Space Science, Department of Physics and Technology, University of Bergen, Bergen, Norway.

出版信息

Nature. 2021 Jan;589(7842):371-375. doi: 10.1038/s41586-020-03122-6. Epub 2021 Jan 20.

Abstract

Blue jets are lightning-like, atmospheric electric discharges of several hundred millisecond duration that fan into cones as they propagate from the top of thunderclouds into the stratosphere. They are thought to initiate in an electric breakdown between the positively charged upper region of a cloud and a layer of negative charge at the cloud boundary and in the air above. The breakdown forms a leader that transitions into streamers when propagating upwards. However, the properties of the leader, and the altitude to which it extends above the clouds, are not well characterized. Blue millisecond flashes in cloud tops have previously been associated with narrow bipolar events, which are 10- to 30-microsecond pulses in wideband electric field records, accompanied by bursts of intense radiation at 3 to 300 megahertz from discharges with short (inferred) channel lengths (less than one kilometre). Here we report spectral measurements from the International Space Station, which offers an unimpeded view of thunderclouds, with 10-microsecond temporal resolution. We observe five intense, approximately 10-microsecond blue flashes from a thunderstorm cell. One flash initiates a pulsating blue jet to the stratopause (the interface between the stratosphere and the ionosphere). The observed flashes were accompanied by 'elves' in the ionosphere. Emissions from lightning leaders in the red spectral band are faint and localized, suggesting that the flashes and the jet are streamer ionization waves, and that the leader elements at their origin are short and localized. We propose that the microsecond flashes are the optical equivalent of negative narrow bipolar events observed in radio waves. These are known to initiate lightning within the cloud and to the ground, and blue lightning into the stratosphere, as reported here.

摘要

蓝色喷流是闪电状的大气电放电,持续时间为数百毫秒,在从雷暴云顶传播到平流层时呈锥形展开。它们被认为是在云的带正电的上部区域和云边界及上方空气中的负电荷层之间的电击穿中产生的。击穿形成一个先导,当向上传播时转变为流光。然而,先导的特性以及它延伸到云层上方的高度并没有很好地表征。云顶的蓝色毫秒闪光以前与窄双极事件有关,窄双极事件是宽带电场记录中 10 到 30 微秒的脉冲,伴随着放电时 3 到 300 兆赫的强烈辐射爆发,放电的通道长度较短(推断)(小于一公里)。在这里,我们报告了国际空间站的光谱测量结果,该站提供了对雷暴云的无障碍观测,具有 10 微秒的时间分辨率。我们观察到一个雷暴单元中有五个强烈的、大约 10 微秒的蓝色闪光。一个闪光引发了一个脉动的蓝色喷流向平流层顶(平流层和电离层之间的界面)。观察到的闪光伴随着电离层中的“小精灵”。在红色光谱带中闪电先导的发射很微弱且局限,表明闪光和喷流是流光电离波,而其起源的先导元素很短且局限。我们提出,微秒闪光是在无线电波中观察到的负窄双极事件的光学等效物。正如这里所报道的,这些事件已知会在云内和地面引发闪电,并向平流层引发蓝色闪电。

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