Lorenz Ralph D
Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Road, Laurel, MD 20723, USA.
Icarus. 2016 Jun;271:326-337. doi: 10.1016/j.icarus.2016.02.001. Epub 2016 Feb 10.
A physically-realistic migrating vortex model is developed and applied to generate pressure and wind speed and direction histories for dust devil passage. The asymmetric character of wind histories is noted, and we examine how these combined data constrain the solution space of dust devil parameters (migration velocity, diameter and intensity), ambient wind, and miss distance. These histories are compared with a new terrestrial field dataset of high-time resolution pressure and wind measurements of over twenty dust devil encounters in New Mexico . This new dataset is made available electronically and it is found that model fits can be typically achieved with simultaneous root-mean-square errors of 0.05 hPa (5-10% of the peak pressure signature), ~20 of wind azimuth, and ~2 m/s windspeed. The fits are not unique, however, and some heuristic aspects of resolving the intrinsic degeneracies of the problem and nonideal features of real encounters are discussed. The application of this approach to the InSight lander is noted, offering the possibility of defining the context for any possible detections of electromagnetic and seismic signatures of dust devils on Mars.
开发了一种物理逼真的迁移涡旋模型,并将其应用于生成尘卷风通过时的压力、风速和风向历史记录。注意到风历史记录的不对称特征,并且我们研究了这些组合数据如何限制尘卷风参数(迁移速度、直径和强度)、环境风以及错过距离的解空间。将这些历史记录与新的地面现场数据集进行比较,该数据集是新墨西哥州二十多次尘卷风遭遇的高时间分辨率压力和风速测量数据。这个新数据集以电子方式提供,并且发现通常可以实现模型拟合,同时均方根误差约为0.05 hPa(约为峰值压力特征的5 - 10%)、风向约为20°以及风速约为2 m/s。然而,这些拟合并非唯一,并且讨论了解决该问题固有简并性和实际遭遇的非理想特征的一些启发式方面。提到了将这种方法应用于洞察号着陆器,这为确定火星上尘卷风的任何可能电磁和地震信号检测的背景提供了可能性。