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Volcanic ash cloud detection from space: a comparison between RSTASH technique and water vapour corrected BTD procedure

机译:从空间探测火山灰云:RsTasH技术与水汽修正BTD程序的比较

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摘要

Volcanic eruptions can inject large amounts (Tg) of gas and particles into thetroposphere and, sometimes, into the stratosphere. Besides the main gases (H2O,CO2, SO2 and HCl), volcanic clouds contain a mix of silicate ash particles in thesize range from 0.1 mm to 1 mm or larger. The interest in volcanic ash detection ishigh, particularly because it represents a serious hazard for air traffic. Particleswith dimensions of several millimetres can damage the aircraft structure(windows, wings, ailerons), while particles less than 10 mm may be extremelydangerous for the jet engines and are undetectable by the pilots during night or inlow visibility conditions. Furthermore, ash detection represents a critical steptowards quantitative retrievals of plume parameters. In this paper two differentsatellite techniques for volcanic cloud detection and tracking are compared,namely a water vapour corrected version of the brightness temperature difference(BTD-WVC) procedure and an implementation of the robust satellite technique,specifically configured for volcanic ash (RSTASH). The BTD method identifiesvolcanic ash clouds on the basis of the brightness temperature differencemeasured in two infrared spectral bands at around 11 and 12 mm. To account forthe atmospheric water vapour differential absorption in the 11–12 mm spectralrange, which tends to reduce (and in some cases completely mask) the BTDsignal, a water vapour correction procedure has been developed (BTD-WVC),based on measured or synthetic atmospheric profiles. RSTASH instead, is based onthe analysis of a time series of satellite records, aimed at identifying signalanomalies through an automatic unsupervised change detection step. To assessthe performance of the BTD-WVC and RSTASH methods in detecting volcanicash clouds, some eruptive events of Mt Etna, observed by the Advanced VeryHigh Resolution Radiometer (AVHRR) sensor, have been analysed. Theobtained results show a good agreement between the BTD-WVC and RSTASHtechniques for all the considered images, in terms of pixels detected as ‘ashaffected’ (i.e. the ash cloud area). In particular, compared to the traditional BTD procedure, the BTD-WVC and RSTASH techniques significantly improve volcanicash cloud detection, both in daytime and night-time data, especially in the case oflow ash loading.
机译:火山喷发会将大量的气体和颗粒注入对流层,有时还会注入到平流层。除主要气体(H2O,CO2,SO2和HCl)外,火山云还包含大小为0.1毫米至1毫米或更大的硅酸盐灰分颗粒混合物。火山灰检测的兴趣很高,特别是因为它对空中交通构成严重危害。几毫米大小的微粒可能会损坏飞机的结构(窗户,机翼,副翼),而小于10毫米的微粒对喷气发动机可能是极为危险的,并且在夜间或低能见度条件下飞行员无法察觉。此外,灰分检测代表了逐步恢复羽状参数的关键步骤。本文比较了两种用于火山云探测和跟踪的不同卫星技术,即水蒸气校正版本的亮温差(BTD-WVC)过程和鲁棒卫星技术的实现,该技术专门针对火山灰(RSTASH)配置。 BTD方法根据在11和12 mm左右的两个红外光谱带中测得的亮度温度差来识别火山灰云。为了解决11-12 mm光谱范围内的大气水汽差异吸收(这往往会降低(在某些情况下完全掩盖)BTDsignal)的问题,已开发了一种基于实测或合成的水汽校正程序(BTD-WVC)大气廓线。 RSTASH则基于对卫星记录的时间序列的分析,旨在通过自动无监督的变化检测步骤来识别信号异常。为了评估BTD-WVC和RSTASH方法在检测火山云中的性能,已经分析了由超高分辨率高分辨率辐射计(AVHRR)传感器观测到的埃特纳火山爆发事件。所获得的结果表明,对于所有考虑的图像,BTD-WVC和RSTASH技术之间都具有良好的一致性,就被检测为“受灰烬影响”的像素(即灰云区域)而言。特别是,与传统的BTD程序相比,BTD-WVC和RSTASH技术在白天和晚上的数据中,尤其是在低灰分负载的情况下,显着改善了火山云的检测。

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