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首页> 外文期刊>Geophysical Research Letters >An ionized layer in the upper atmosphere of Mars caused by dust impacts from comet Siding Spring
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An ionized layer in the upper atmosphere of Mars caused by dust impacts from comet Siding Spring

机译:火星上层大气的电离层是由彗星壁板弹簧的尘埃撞击引起的

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We report the detection of a dense ionized layer in the upper atmosphere of Mars caused by the impact of dust from comet Siding Spring. The observations were made by the ionospheric radar sounder on the Mars Express spacecraft during two low-altitude passes approximately 7h and 14h after closest approach of the comet to Mars. During these passes an unusual transient layer of ionization was detected at altitudes of about 80 to 100km with peak electron densities of (1.5 to 2.5)x10(5)cm(-3), much higher than normally observed in the Martian ionosphere. From comparisons to previously observed ionization produced by meteors at Earth and Mars, we conclude that the layer was produced by dust from the comet impacting and ionizing the upper atmosphere of Mars.
机译:我们报告了探测到的火星上层大气中一个密集的电离层,这是由来自Siding Spring彗星的尘埃的影响引起的。观测是由火星快车上的电离层雷达测深仪在距彗星最接近火星的大约7h和14h进行两次低空飞行时进行的。在这些通过过程中,在约80至100 km的高度上检测到一个异常的电离瞬变层,其峰值电子密度为(1.5至2.5)x10(5)cm(-3),远高于火星电离层中的正常观测值。通过与之前观测到的流星在地球和火星上产生的电离的比较,我们得出结论,该层是由彗星撞击和电离火星上层大气的尘埃产生的。

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