{"id":31443,"date":"2022-10-26T10:31:14","date_gmt":"2022-10-26T08:31:14","guid":{"rendered":"https:\/\/karmaka.de\/?p=31443"},"modified":"2022-10-26T10:31:15","modified_gmt":"2022-10-26T08:31:15","slug":"methode-des-rayons-complexes-pour-la-propagation-infrasonore-application-au-bang-sonique-dun-meteoroide","status":"publish","type":"post","link":"https:\/\/karmaka.de\/?p=31443","title":{"rendered":"M\u00e9thode des rayons complexes pour la propagation infrasonore. Application au bang sonique d\u2019un m\u00e9t\u00e9oro\u00efde"},"content":{"rendered":"\n<p>Annie Zelias<\/p>\n\n\n\n<p>PhD thesis (in French)<\/p>\n\n\n\n<p><a href=\"https:\/\/tel.archives-ouvertes.fr\/tel-03828809\/document\" target=\"_blank\" rel=\"noreferrer noopener\"><strong>PDF (OPEN ACCESS)<\/strong><\/a><\/p>\n\n\n\n<p class=\"justify-text\">Most of high-energy atmospheric phenomena, either natural (meteoroids, earthquakes, volcanoes, etc.) or anthropogenic (aircraft, chemical or nuclear explosions, etc.) emit acoustic waves of frequencies lower than 20 Hz, called infrasound. These waves can spread over thousands of kilometers thanks to their low attenuation and to the atmosphere stratification that guides their propagation. These long distances allow observation of acoustic information at any time and any point of the Earth. Thus, infrasound constitutes one of the detection technologies used within the framework of the Compehensive Nuclear-Test-Ban Treaty (CTBT). Simulation of the infrasonic propagation is the topic of many studies, in particular by parabolic approaches, finite difference models, eigen modes summations or by asymptotic methods such as ray tracing. This last one is suitable at a low numerical cost for very long distances in an inhomogeneous and advected medium, in three dimensions and for nonlinear effects. However, this method remains limited by the presence of caustics and shadow zones for which it is singular. In order to predict the geometrical parameters and the pressure signatures in these zones, while keeping its efficiency, we adapt the complex ray tracing method to the atmospheric propagation of infrasound.<br>In a first step, the usual ray method is recalled and its extension to the complex plane is presented. An analytical application is treated, corresponding to a fold horizontal caustic above the ground which can be formed by a supersonic flight at low Mach. This case highlights the influence of complex rays reflection on the ground, depending on the caustic altitude. In a second step, we develop a two-dimensional numerical algorithm computing eigenrays (rays<br>directly connecting the source to the receivers) in the whole domain and for all arrivals formed by the atmospheric waveguides. A detailed study of the point source case, representative for an explosion, with a reference atmospheric profile complemented by a horizontal wind, allows us to validate the developed eigenray research algorithm, by comparison to the parabolic approximation. The application is extended to the case of a range dependent profile. The<br>neighborhood of caustics is treated by the asymptotic Uniform Theory of Diffraction. For realistic atmospheric profiles, sound speed and wind datas have to be fitted by analytical functions ; various ways of fitting are proposed and compared to one another. This is then applied to a simplified case, inspired by the Carancas meteorite observed on September 15, 2007 in Peru. The outputs of the complex ray theory are compared to the recorded datas at one infrasound station located in the shadow zone. This shows that the complex ray method is effective in determining the geometrical parameters in the shadow zones.<\/p>\n\n\n\n<p class=\"justify-text\">&#8220;R\u00e9sum\u00e9 : La plupart des ph\u00e9nom\u00e8nes atmosph\u00e9riques de forte \u00e9nergie, qu&#8217;ils soient naturels ou anthropiques \u00e9mettent des ondes de fr\u00e9quence inf\u00e9rieure \u00e0 20Hz, appel\u00e9es infrasons. Ces ondes peuvent se propager sur des milliers de kilom\u00e8tres en b\u00e9n\u00e9ficiant de leur faible att\u00e9nuation et de la structure de l&#8217;atmosph\u00e8re qui guide leur propagation. Dans le but de pr\u00e9dire les param\u00e8tres g\u00e9om\u00e9triques et les signatures dans les zones d&#8217;ombres, nous avons adapt\u00e9 la m\u00e9thode des rayons complexes \u00e0 la propagation atmosph\u00e9rique des infrasons. Pour cela nous avons d\u00e9velopp\u00e9 une m\u00e9thode num\u00e9rique permettant de calculer les rayons propres dans tout le domaine. Une \u00e9tude d\u00e9taill\u00e9e sur le cas d&#8217;une source ponctuelle, analogue \u00e0 une explosion a permis de valider l&#8217;algorithme par une comparaison \u00e0 une m\u00e9thode d&#8217;approximation parabolique. Une m\u00e9thodologie d&#8217;ajustement de donn\u00e9es de vitesse du son et du vent par des fonctions analytiques a \u00e9t\u00e9 mise en place, afin de permettre l&#8217;utilisation de profils atmosph\u00e9riques r\u00e9alistes adapt\u00e9s \u00e0 la m\u00e9thode des rayons complexes. Cela a donn\u00e9 lieu \u00e0 l&#8217;application \u00e0 un cas simplifi\u00e9 de m\u00e9t\u00e9orite (m\u00e9t\u00e9orite de Carancas observ\u00e9e le 15 septembre 2007 au P\u00e9rou), dont les signatures ont \u00e9t\u00e9 enregistr\u00e9es par une station infrasonore localis\u00e9e en zone d&#8217;ombre. Ce cas nous a permis de montrer l&#8217;efficacit\u00e9 de la m\u00e9thode des rayons complexes. &#8220;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Annie Zelias PhD thesis (in French) PDF (OPEN ACCESS) Most of high-energy atmospheric phenomena, either natural (meteoroids, earthquakes, volcanoes, etc.) or anthropogenic (aircraft, chemical or nuclear explosions, etc.) emit acoustic waves of frequencies lower than&#8230;<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[96,97],"tags":[303,1380,3716,226,3187,98,4173,3715,141,1832],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/31443"}],"collection":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=31443"}],"version-history":[{"count":1,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/31443\/revisions"}],"predecessor-version":[{"id":31444,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/31443\/revisions\/31444"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=31443"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=31443"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=31443"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}