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来自新西兰的SAR弧线

(原标题: A SAR Arc from New Zealand)

2024-01-03

浏览次数: 17

环绕在极光周围的不寻常的红色光环是什么?它是一个稳定的极光红(SAR)弧。SAR弧是罕见的,自1954年以来才被承认和研究。这张特色的广角照片几乎捕捉到了整个围绕着更常见的绿色和红色极光的SAR弧线,拍摄于本月早些时候在新西兰普尔本,当时正值一场特别强烈的地磁风暴。SAR弧形成的原因仍然是一个研究课题,但很可能与地球的保护磁场有关,这是一个由地球深处的熔融铁流动产生的磁场。这个磁场通常会将来自太阳风的带电粒子重新定向到地球两极。然而,它也在靠近赤道的地方捕获了一圈离子,在太阳活动频繁的时候,它们可以从磁层中获得能量。这个离子环中的高能电子可以与地球电离层中比典型极光更高的氧气碰撞并激发氧气,导致氧气发出红光。正在进行的研究发现,红色的SAR弧线甚至可以转变成紫色和绿色的STEVE弧线。

查看原文解释

What is that unusual red halo surrounding this aurora? It is a Stable Auroral Red (SAR) arc. SAR arcs are rare and have only been acknowledged and studied since 1954. The featured wide-angle photograph, capturing nearly an entire SAR arc surrounding more common green and red aurora, was taken earlier this month from Poolburn, New Zealand, during an especially energetic geomagnetic storm. Why SAR arcs form remains a topic of research, but is likely related to Earth's protective magnetic field, a field created by molten iron flowing deep inside the Earth. This magnetic field usually redirects incoming charged particles from the Sun's wind toward the Earth's poles. However, it also traps a ring of ions closer to the equator, where they can gain energy from the magnetosphere during high solar activity. The energetic electrons in this ion ring can collide with and excite oxygen higher in Earth's ionosphere than typical auroras, causing the oxygen to glow red. Ongoing research has uncovered evidence that a red SAR arc can even transform into a purple and green STEVE.

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