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Odin-OSIRIS detection of the Chelyabinsk meteor

机译:Odin-OSIRIS检测车里雅宾斯克流星

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On 15 February 2013 an 11000 ton meteor entered Earth's atmosphere southeast of Chelyabinsk, creating a large fireball at 23 km altitude. The resulting stratospheric aerosol loading was detected by the Ozone Mapping and Profiler Suite (OMPS) in a high-altitude polar belt. This work confirms the presence and lifetime of the stratospheric debris using the Optical Spectrograph and InfraRed Imaging System (OSIRIS) onboard the Odin satellite. Although OSIRIS coverage begins in mid-March, the measurements show a belt of enhanced scattering near 35 km altitude between 50° N and 70° N. Initially, enhancements show increased scattering of up to 15 % over the background conditions, decaying in intensity and dropping in altitude until they are indistinguishable from background conditions by mid-May. An inversion is also attempted using the standard OSIRIS processing algorithm to determine the extinction in the meteoric debris.
机译:2013年2月15日,一颗11000吨的流星进入车里雅宾斯克东南部的地球大气层,在23公里的高度处制造了一个大型火球。在高海拔极地带中,臭氧平测仪和纵剖面仪套件(OMPS)探测到了由此产生的平流层气溶胶负荷。这项工作使用Odin卫星上的光谱仪和红外成像系统(OSIRIS)确认了平流层碎片的存在和寿命。尽管OSIRIS的覆盖范围从3月中旬开始,但测量显示在35°高度在50°N和70°N之间的35 km高度附近散射增强。最初,增强显示在背景条件下散射增加高达15%,强度和强度衰减。直到5月中旬与背景条件无法区分为止。还尝试使用标准OSIRIS处理算法进行反演,以确定陨石碎片的灭绝。

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