首页> 外文期刊>Journal of atmospheric and solar-terrestrial physics >Space shuttle exhaust plumes in the lower thermosphere: Advective transport and diffusive spreading
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Space shuttle exhaust plumes in the lower thermosphere: Advective transport and diffusive spreading

机译:低空热层中的航天飞机尾气羽流:正向运输和扩散扩散

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The space shuttle main engine plume deposited between 100 and 115 km altitude is a valuable tracer for global-scale dynamical processes. Several studies have shown that this plume can reach the Arctic or Antarctic to form bursts of polar mesospheric clouds (PMCs) within a few days. The rapid transport of the shuttle plume is currently not reproduced by general circulation models and is not well understood. To help delineate the issues, we present the complete satellite datasets of shuttle plume observations by the Sounding of the Atmosphere using Broadband Emission Radiometry instrument and the Sub- Millimeter Radiometer instrument. From 2002 to 2011 these two instruments observed 27 shuttle plumes in over 600 limb scans of water vapor emission, from which we derive both advective meridional transport and diffusive spreading. Each plume is deposited at virtually the same place off the United States east coast so our results are relevant to northern mid-latitudes. We find that the advective transport for the first 6-18 h following deposition depends on the local time (LT) of launch: shuttle plumes deposited later in the day (~ 13-22 LT) typically move south whereas they otherwise typically move north. For these younger plumes rapid transport is most favorable for launches at 6 and 18 LT, when the displacement is 10° in latitude corresponding to an average wind speed of 30 m/s. For plumes between 18 and 30 h old some show average sustained meridional speeds of 30 m/s. For plumes between 30 and 54 h old the observations suggest a seasonal dependence to the meridional transport, peaking near the beginning of year at 24 m/s. The diffusive spreading of the plume superimposed on the transport is on average 23 m/s in 24 h. The plume observations show large variations in both meridional transport and diffusive spreading so that accurate modeling requires knowledge of the winds specific to each case. The combination of transport and spreading from the STS-118 plume in August 2007 formed bright PMCs between 75 and 85°N a day after launch. These are the highest latitude Arctic PMCs formed by shuttle exhaust reported to date.
机译:沉积在100至115 km高度之间的航天飞机主发动机羽流是全球动态过程的重要示踪剂。多项研究表明,这种羽流可以在几天内到达北极或南极,形成极地中层云(PMC)爆发。穿梭羽流的快速运输目前还没有被一般的循环模型所再现,也没有被很好地理解。为帮助描述问题,我们使用宽带发射辐射仪和亚毫米辐射仪,通过大气探测,提供了航天飞机羽流观测的完整卫星数据集。从2002年到2011年,这两种仪器在600多条水蒸气排放的肢体扫描中观测到27个航天飞机羽流,从中我们得出对流子午线运输和扩散扩散。每个羽流几乎都沉积在美国东海岸附近的同一地点,因此我们的结果与北部中纬度有关。我们发现沉积后头6-18小时的平流运输取决于发射的当地时间(LT):当天晚些时候沉积的梭羽(〜13-22 LT)通常向南移动,否则通常向北移动。对于这些较年轻的羽流,当位移为纬度10°(相当于30 m / s的平均风速)时,最适合在6和18 LT发射。对于年龄在18至30小时之间的羽流,某些子午流显示出平均持续经向速度为30 m / s。对于30至54小时之间的羽流,观测结果表明对子午线运输的季节性依赖性,在年初接近24 m / s时达到峰值。叠加在运输装置上的羽流的扩散扩散在24小时内平均为23 m / s。羽流观测结果表明,子午向传输和扩散扩散都存在较大差异,因此要进行精确的建模,需要了解每种情况下特定的风。 STS-118烟羽在2007年8月的运输和扩散相结合,形成了发射后一天介于75和85°N之间的明亮PMC。这是迄今为止报道的航天飞机尾气形成的最高纬度北极PMC。

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