{"id":578,"date":"2026-01-07T16:21:13","date_gmt":"2026-01-07T16:21:13","guid":{"rendered":"https:\/\/paris-remote-sensing-master.fr\/?page_id=578"},"modified":"2026-02-24T17:24:39","modified_gmt":"2026-02-24T17:24:39","slug":"syllabus","status":"publish","type":"page","link":"https:\/\/paris-remote-sensing-master.fr\/?page_id=578","title":{"rendered":"Syllabus"},"content":{"rendered":"\n<div id=\"M2\" class=\"wp-block-group is-layout-constrained wp-block-group-is-layout-constrained\">\n<h2 class=\"wp-block-heading\">Tronc commun &#8211; 54 ECTS<\/h2>\n\n\n\n<div style=\"height:50px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-28f84493 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column has-background is-layout-flow wp-block-column-is-layout-flow\" style=\"background-color:#00690014;padding-top:var(--wp--preset--spacing--30);padding-right:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--30);padding-left:var(--wp--preset--spacing--30)\">\n<h3 class=\"wp-block-heading\">Rayonnement \u00e9lectromagn\u00e9tique &#8211; 3 ECTS<\/h3>\n\n\n\n<p>Responsable UE : Shermila Mostarshedi<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>En savoir plus<\/summary>\n<h4 class=\"wp-block-heading\">Propagation des ondes<\/h4>\n\n\n\n<p>Professeur : Shermila Mostarshedi<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Aper\u00e7u<\/summary>\n<p>Ce cours pr\u00e9sente les \u00e9quations fondamentales de l&#8217;\u00e9lectromagn\u00e9tisme et les concepts qui en d\u00e9coulent.<\/p>\n\n\n\n<ul class=\"wp-block-list\">\n<li>Rappel de calcul vectoriel<\/li>\n\n\n\n<li>Equations et relations fondamentales en \u00e9lectromagn\u00e9tisme : \u00e9quations de Maxwell, pr\u00e9sentation int\u00e9grale des \u00e9quations de Maxwell, conditions aux limites, relations constitutives, consid\u00e9rations \u00e9nerg\u00e9tiques et vecteur de Poynting, potentiels retard\u00e9s et fonctions de Green<\/li>\n\n\n\n<li>Electromagn\u00e9tisme en r\u00e9gime harmonique : \u00e9quations de Maxwell et conditions aux limites en r\u00e9gime harmonique, relations constitutives en r\u00e9gime harmonique et permittivit\u00e9 complexe, permittivit\u00e9 des mat\u00e9riaux di\u00e9lectriques et des mat\u00e9riaux conducteurs, relations de dispersion de Kramers-Kr\u00f6nig<\/li>\n\n\n\n<li>Ondes planes en r\u00e9gime harmonique : composantes des champs en r\u00e9gime harmonique, \u00e9quation de Helmholtz sans second membre pour un milieu LIH, ondes planes dans un milieu absorbant, ondes planes dans un milieu absorbant, puissance \u00e9lectromagn\u00e9tique en r\u00e9gime harmonique<\/li>\n\n\n\n<li>Ondes sph\u00e9riques &#8211; Rayonnement d\u2019une antenne en r\u00e9gime harmonique : relations d\u2019orthogonalit\u00e9 \u00e0 grande distance de la source, surfaces \u00e9quiphases et ondes sph\u00e9riques, vecteur de Poynting d\u2019une onde sph\u00e9rique dans un milieu non absorbant, polarisation des ondes<\/li>\n\n\n\n<li>Faisceaux d\u2019ondes planes : constantes de propagation d\u2019une onde plane, ondes planes \u00e9vanescentes et propagatives dans un milieu sans pertes, ondes planes \u00e9vanescentes dans un milieu avec pertes, faisceau d\u2019ondes planes 3D, faisceau d\u2019ondes planes 2D, comportement asymptotique d\u2019un faisceau d\u2019ondes planes, d\u00e9polarisation des ondes par une surface, diffraction par une surface rugueuse et hypoth\u00e8se de Rayleigh<\/li>\n\n\n\n<li>Propagation dans diff\u00e9rents types de milieux<\/li>\n\n\n\n<li>Principe d\u2019\u00e9quivalence, application \u00e0 la diffraction des ouvertures<\/li>\n\n\n\n<li>Etude des surfaces p\u00e9riodiques, application \u00e0 la r\u00e9flexion des surfaces rugueuses<\/li>\n\n\n\n<li>TD1 : des \u00e9quations de Maxwell aux conditions aux limites<\/li>\n\n\n\n<li>TD2 : permittivit\u00e9 complexe des mat\u00e9riaux<\/li>\n\n\n\n<li>TD3 : ondes planes et Ondes sph\u00e9riques<\/li>\n\n\n\n<li>TD4 : \u00e9tude d\u2019un faisceau gaussien (2D)<\/li>\n\n\n\n<li>TD5: comportement asymptotique d\u2019un faisceau d\u2019ondes planes 2D<\/li>\n\n\n\n<li>TD6 : champ diffract\u00e9 par une surface &#8211; Bilan de puissance<\/li>\n<\/ul>\n<\/details>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Bibliographie<\/summary>\n<ul class=\"wp-block-list\">\n<li>Born M., Wolf E. (1999),&nbsp;<em>Principles of optics: Electromagnetic Theory of Propagation, Interference and Diffraction of Light<\/em>, Cambridge University Press, 985 pp.<\/li>\n\n\n\n<li>Ishimaru A. (1990),&nbsp;<em>Electromagnetic Wave Propagation, Radiation and Scattering<\/em>, Prentice Hall, 656 pp.<\/li>\n\n\n\n<li>Petit R. (1997),&nbsp;<em>Ondes \u00e9lectromagn\u00e9tiques en radio\u00e9lectricit\u00e9 et en optique<\/em>, Dunod, 349 pp.<\/li>\n\n\n\n<li>Stratton J.A. (2007),&nbsp;<em>Electromagnetic theory<\/em>, Wiley-IEEE Press, 640 pp.<\/li>\n<\/ul>\n<\/details>\n\n\n\n<h4 class=\"wp-block-heading\">Dispersion des ondes \u00e9lectromagn\u00e9tiques<\/h4>\n\n\n\n<p>Professeur : Eric Pantin<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Aper\u00e7u<\/summary>\n<p>Cette conf\u00e9rence traite du rayonnement \u00e9lectromagn\u00e9tique \u00e9mis dans l&#8217;espace libre et en pr\u00e9sence d&#8217;objets diffractants. Elle s&#8217;appuie principalement sur l&#8217;\u00e9quation int\u00e9grale du champ \u00e9lectrique.<\/p>\n\n\n\n<p>Partie I : Propagation des OEM<\/p>\n\n\n\n<ul class=\"wp-block-list\">\n<li>Rayonnement de sources en espace libre<br>&#8211; rappels des equations de Maxwell et conditions d&#8217;application<br>&#8211; \u00e9quations de maxwell en r\u00e9gime harmonique<br>&#8211; relations de continuit\u00e9<br>&#8211; \u00e9quations de Helmholtz<br>&#8211; r\u00e9solution des \u00e9quations de propagation en espace libre en pr\u00e9sence de sources<\/li>\n\n\n\n<li>OEM en pr\u00e9sence d&#8217;obstacles<br>&#8211; Principe d&#8217;\u00e9quivalence de Rayleigh-Gans et r\u00e9solution des \u00e9quations<\/li>\n\n\n\n<li>Diffraction par une surface<br>&#8211; plane infinie<br>&#8211; plane limit\u00e9e<br>&#8211; non-plane<\/li>\n\n\n\n<li>Diffusion\/absorption\/\u00e9mission par des particules<br>&#8211; principe de r\u00e9solution<br>&#8211; solutions de Mie\/limites optique g\u00e9om\u00e9trique<br>&#8211; approximation de Rayleigh-Gans<br>&#8211; Qabs\/Qsca\/Qext, param\u00e8tre d&#8217;assym\u00e9trie, fonction de phase<br>&#8211; cons\u00e9quences et cas pratique<\/li>\n<\/ul>\n\n\n\n<p>Partie II : interaction mati\u00e8re-ondes EM<\/p>\n\n\n\n<ul class=\"wp-block-list\">\n<li>Mod\u00e8les de Drude et Lorentz<\/li>\n\n\n\n<li>Mod\u00e8le de Debye<\/li>\n\n\n\n<li>Relations de Kramers-Kr\u00f6nig<\/li>\n\n\n\n<li>R\u00e8gles de m\u00e9lange Maxwell-Garnett et Bruggemann<\/li>\n<\/ul>\n<\/details>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Bibliographie<\/summary>\n<ul class=\"wp-block-list\">\n<li>Beckmann A. &amp; Spizzichino A. (1987),&nbsp;<em>The scattering of electromagnetic waves from rough surfaces<\/em>, Artech House Radar Library, 512 pp.<\/li>\n\n\n\n<li>Born M. &amp; Wolf E. (1999), <em>Principles of optics: Electromagnetic theory of propagation, interference and diffraction of light<\/em>, Cambridge University Press, 985 pp.<\/li>\n\n\n\n<li>Brekhovski L.M. &amp; Godin O.A. (1998),&nbsp;<em>Acoustics of Layered Media I: Plane and Quasi-Plane Waves<\/em>, Springer, 250 pp.<\/li>\n\n\n\n<li>Chew W.C. (1999),&nbsp;<em>Waves and Fields in Inhomogeneous Media<\/em>, Wiley-IEEE Press, 632 pp.<\/li>\n\n\n\n<li>Dassios G. &amp; Kleinman R. (2000),&nbsp;<em>Low Frequency Scattering<\/em>, Oxford University Press, 320 pp.<\/li>\n\n\n\n<li>Fournet G. (1979), <em>Electromagn\u00e9tisme : \u00e0 partir des \u00e9quations locales<\/em>, Masson, 478 pp.<\/li>\n\n\n\n<li>Ishimaru A. (1999),&nbsp;<em>Waves Propagation and Scattering in Random Media<\/em>, Wiley-IEEE Press, 600 pp.<\/li>\n\n\n\n<li>Kaufman A.A. &amp; Keller G.V. (1985),&nbsp;<em>Inductive Mining Prospecting, Part 1: Theory<\/em>, Elsevier, 617 pp.<\/li>\n\n\n\n<li>Kong J.A. (1986),&nbsp;<em>Electromagnetic Wave Theory<\/em>, John Wiley &amp; Sons Inc, 710 pp.<\/li>\n\n\n\n<li>Petit R. (2011).&nbsp;<em>Electromagnetic Theory of Gratings<\/em>, Springer, 304 pp.<\/li>\n\n\n\n<li>Roubine E. &amp; Bolomey J.C. (1978),&nbsp;<em>Antennes &#8211; Tome I,<\/em>&nbsp;Masson, 2020 pp.<\/li>\n\n\n\n<li>Tai C.T. (1994),&nbsp;<em>Dyadic Green Function in Electromagnetic Theory<\/em>, IEEE, 343 pp.<\/li>\n<\/ul>\n<\/details>\n\n\n\n<h4 class=\"wp-block-heading\">Ondes acoustiques<\/h4>\n\n\n\n<p>Professeur : Didier Cassereau<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Aper\u00e7u<\/summary>\n<p>Cette conf\u00e9rence pr\u00e9sente les principes fondamentaux de la propagation monochromatique et transitoire des ondes acoustiques dans les milieux fluides.<\/p>\n\n\n\n<ul class=\"wp-block-list\">\n<li>El\u00e9ments d\u2019acoustique physique : introduction, sources sonores, r\u00e9cepteurs, fr\u00e9quence des ondes acoustiques, niveau sonore, vitesse de propagation, polarisation des ondes acoustiques, ondes acoustiques dans les milieux fluides, r\u00e9solution de l\u2019\u00e9quation d\u2019ondes \u00e0 une dimension, imp\u00e9dance acoustique, propagation dans un espace \u00e0 trois dimensions<\/li>\n\n\n\n<li>R\u00e9flexion et transmission des ondes acoustiques : introduction, syst\u00e8mes lin\u00e9aires et invariants partranslation, r\u00e9flexion d\u2019une onde acoustique sur une paroi rigide, r\u00e9flexion d\u2019une onde acoustique sur une paroi molle, dioptre acoustique, approximation g\u00e9om\u00e9trique de la transmission, application au calcul de fronts d\u2019onde, r\u00e9flexion et transmission par deux interface parall\u00e8les<\/li>\n\n\n\n<li>Th\u00e9orie du signal \u00e0 deux dimensions : introduction, rappels, th\u00e9orie du signal en acoustique, \u00e9tude des exponentielles complexes<\/li>\n\n\n\n<li>Th\u00e9orie scalaire de la diffraction : introduction, diffraction par un \u00e9cran plan, diffraction transitoire<\/li>\n\n\n\n<li>Diffraction de Fresnel et Fraunhofer : introduction, premi\u00e8res approximations, approximation de Fresnel, approximation de Fraunhofer, exemples de diffraction de Fraunhofer<\/li>\n\n\n\n<li>Diffraction impulsionnelle par un piston circulaire : formalisme impulsionnel de la diffraction, application au cas du piston circulaire<\/li>\n<\/ul>\n<\/details>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Bibliographie<\/summary>\n<ul class=\"wp-block-list\">\n<li>Brekhovskikh L.M. (1980),&nbsp;<em>Waves in layered media<\/em>, Academic Press, 503 pp.<\/li>\n\n\n\n<li>Brekhovskikh L.M., Goncharov V.V. (1985),&nbsp;<em>Mechanics of continua and wave dynamics<\/em>, Springer-Verlag, 342 pp.<\/li>\n\n\n\n<li>Bruneau M.(1998),&nbsp;<em>Manuel d&#8217;acoustique fondamentale<\/em>, Hermes Science Publications, 576 pp.<\/li>\n\n\n\n<li>Davis J.L. (1988),&nbsp;<em>Wave propagation in solids and fluids<\/em>, Springer-Verlag, 386 pp.<\/li>\n\n\n\n<li>Filippi P., Collectif (1994),&nbsp;<em>Acoustique g\u00e9n\u00e9rale<\/em>, Editions de Physique , 371 pp.<\/li>\n\n\n\n<li>Goodman J.W. (1968),&nbsp;<em>Introduction to Fourier optics<\/em>, McGraw-Hill, 287 pp.<\/li>\n\n\n\n<li>Gordon S.K. (1987),&nbsp;<em>Acoustic waves: Devices, imaging, and analog signal processing<\/em>, Prentice Hall, 601 pp.<\/li>\n\n\n\n<li>2Guyader J.L. (2002),&nbsp;<em>Vibrations des milieux continus<\/em>, Hermes Science Publications, 445 pp.<\/li>\n\n\n\n<li>Royer D., Dieulesaint E. (1999),&nbsp;<em>Ondes \u00e9lastiques dans les solides. Tome 2 . G\u00e9n\u00e9ration, interaction acousto-optique, applications<\/em>, Masson, 410 pp..<\/li>\n<\/ul>\n<\/details>\n\n\n\n<h4 class=\"wp-block-heading\">Th\u00e9orie des probl\u00e8mes inverses<\/h4>\n\n\n\n<p>Professeur : Nobuaki Fuji<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Bibliographie<\/summary>\n<ul class=\"wp-block-list\">\n<li>Tarantola A. (2005),&nbsp;<em>Inverse problem theory and methods for model parameter estimation<\/em>, Siam, 342 pp.<\/li>\n<\/ul>\n<\/details>\n<\/details>\n<\/div>\n\n\n\n<div class=\"wp-block-column has-background is-layout-flow wp-block-column-is-layout-flow\" style=\"background-color:#00690014;padding-top:var(--wp--preset--spacing--30);padding-right:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--30);padding-left:var(--wp--preset--spacing--30)\">\n<h3 class=\"wp-block-heading\">Stages et s\u00e9minaires &#8211; 3 ECTS<\/h3>\n\n\n\n<p>Responsable UE : S\u00e9bastien Rodriguez<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>En savoir plus<\/summary>\n<div class=\"wp-block-group is-layout-constrained wp-block-group-is-layout-constrained\">\n<p>Professeurs : S\u00e9bastien Rodriguez &amp; H\u00e9l\u00e8ne Chepfer<br>Organisation : Stage de master (4 mois minimum) en laboratoire ou entreprise. En compl\u00e9ment, s\u00e9rie de s\u00e9minaires obligatoires au cours de l&#8217;ann\u00e9e.<\/p>\n<\/div>\n<\/details>\n<\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-28f84493 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column has-background is-layout-flow wp-block-column-is-layout-flow\" style=\"background-color:#00690014;padding-top:var(--wp--preset--spacing--30);padding-right:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--30);padding-left:var(--wp--preset--spacing--30)\">\n<h3 class=\"wp-block-heading\">Image processing &#8211; 3 ECTS<\/h3>\n\n\n\n<p>Responsable UE : Sophie Coustance<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>En savoir plus<\/summary>\n<p>Les satellites d\u2019observation de la terre ont de multiples applications (cartographie, m\u00e9t\u00e9orologie, \u00e9tudes environnementales, urbanisation, d\u00e9fense). Ils permettent depuis l\u2019espace de disposer de couvertures globales et d\u2019observations long terme.<\/p>\n\n\n\n<p>Dans ce cours, on s\u2019int\u00e9ressera au domaine optique (0.4-15\u00b5m). Dans une premi\u00e8re partie, on introduit la physique de la mesure des syst\u00e8mes de t\u00e9l\u00e9d\u00e9tection optique : d\u00e9finition des grandeurs radiatives (luminance, \u00e9clairement), des propri\u00e9t\u00e9s de surface (r\u00e9flectance de surface, effet directionnel, \u00e9missivit\u00e9), de la polarisation et de l\u2019impact de l\u2019atmosph\u00e8re sur le signal parvenant au satellite.<\/p>\n\n\n\n<p>Dans un deuxi\u00e8me temps, l\u2019architecture des syst\u00e8mes de t\u00e9l\u00e9d\u00e9tection optique est pr\u00e9sent\u00e9e.Ils se classent en trois cat\u00e9gories adressant diff\u00e9rents besoins : les radiom\u00e8tres qui privil\u00e9gient la r\u00e9solution radiom\u00e9trique, les spectrom\u00e8tres la r\u00e9solution spectrale et les imageurs ou les interf\u00e9rom\u00e8tres la r\u00e9solution spatiale. Diff\u00e9rents syst\u00e8mes d\u2019acquisition existent : scanner, push- broom, matriciels. L\u2019architecture g\u00e9n\u00e9rale se compose d\u2019un syst\u00e8me collecteur (t\u00e9lescope, lentille), d\u2019un syst\u00e8me de s\u00e9lection spectrale (filtres, prismes), de d\u00e9tecteurs, de syst\u00e8mes de digitalisation et de traitements bord.<\/p>\n\n\n\n<p>Dans un troisi\u00e8me temps, on pr\u00e9sente les corrections et \u00e9talonnages appliqu\u00e9s aux images satellites. Les traitements g\u00e9om\u00e9triques corrigent les perturbations dues aux vibrations du satellite et permettent de d\u00e9terminer les coordonn\u00e9es terrestres des pixels de l\u2019image. L\u2019\u00e9galisation radiom\u00e9trique corrige des diff\u00e9rences de r\u00e9ponse entre les d\u00e9tecteurs. L\u2019\u00e9talonnage absolu permet ensuite de remonter \u00e0 la grandeur physique. Il peut s\u2019effectuer gr\u00e2ce \u00e0 diff\u00e9rentes m\u00e9thodes (comparaisons d\u2019acquisitions entre un satellite \u00e0 \u00e9talonner et un autre servant de r\u00e9f\u00e9rence, acquisitions de la lune, comparaisons avec des mesures in-situ). La qualit\u00e9 radiom\u00e9trique apr\u00e8s ces \u00e9talonnages peut \u00eatre \u00e9valu\u00e9e, elle traduit les performances du syst\u00e8me. On s\u00e9pare cette qualit\u00e9 radiom\u00e9trique en deux crit\u00e8res : la r\u00e9solution radiom\u00e9trique et la pr\u00e9cision d\u2019\u00e9talonnage.<\/p>\n\n\n\n<p>On aborde ensuite la notion de lumi\u00e8re parasite, de sa caract\u00e9risation et des corrections pouvant \u00eatre mises en place avec l\u2019exemple du satellite Ven\u00b5s.<\/p>\n\n\n\n<p>En conclusion, on pr\u00e9sente diff\u00e9rents syst\u00e8mes satellites : 3MI, Pl\u00e9iades, Sentinel-2, etc<\/p>\n<\/details>\n<\/div>\n\n\n\n<div class=\"wp-block-column has-background is-layout-flow wp-block-column-is-layout-flow\" style=\"background-color:#00690014;padding-top:var(--wp--preset--spacing--30);padding-right:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--30);padding-left:var(--wp--preset--spacing--30)\">\n<h3 class=\"wp-block-heading\">Travaux pratiques &#8211; 3 ECTS<\/h3>\n\n\n\n<p>Responsable UE : S\u00e9bastien Rodriguez<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>En savoir plus<\/summary>\n<p>\u00c9quipe p\u00e9dagogique : Ir\u00e8ne Xueref, H\u00e9l\u00e8ne Chepfer, S\u00e9bastien Rodriguez, Julien Jumelet, A. Pazmino, Yao-Veng T\u00e9, Ha Tran, Samuel Nahmani, Rodolphe Marion, Manon Dalaison<\/p>\n\n\n\n<p>L&#8217;ensemble de TP propos\u00e9s ici aux \u00e9tudiants a pour objectif de fournir un large panel de comp\u00e9tences en r\u00e9alisation, traitement et analyse de donn\u00e9es r\u00e9elles d&#8217;observation satellitaire et de m\u00e9thodes g\u00e9ophysiques d&#8217;observation pour la caract\u00e9risation de l&#8217;atmosph\u00e8re et la surface de la Terre et des plan\u00e8tes.<\/p>\n<\/details>\n<\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-28f84493 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column has-background is-layout-flow wp-block-column-is-layout-flow\" style=\"background-color:#00690014;padding-top:var(--wp--preset--spacing--30);padding-right:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--30);padding-left:var(--wp--preset--spacing--30)\">\n<h3 class=\"wp-block-heading\">Transfert radiatif dans l&#8217;atmosph\u00e8re &#8211; 3 ECTS<\/h3>\n\n\n\n<p>Responsable : Cyril Crevoisier<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>En savoir plus<\/summary>\n<h4 class=\"wp-block-heading\">Spectroscopie mol\u00e9culaire<\/h4>\n\n\n\n<p>Professeur : S\u00e9bastien Payan<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Aper\u00e7u<\/summary>\n<p>La spectroscopie mol\u00e9culaire est une m\u00e9thode cl\u00e9 pour d\u00e9terminer la signature spectrale de la Terre et des autres plan\u00e8tes du syst\u00e8me solaire, ainsi que des exoplan\u00e8tes. Elle vise \u00e0 enregistrer le rayonnement \u00e9lectromagn\u00e9tique r\u00e9fl\u00e9chi ou \u00e9mis par une cible (surface ou atmosph\u00e8re) dans des bandes de fr\u00e9quences tr\u00e8s \u00e9troites. Elle joue notamment un r\u00f4le essentiel dans la surveillance de l&#8217;\u00e9volution de notre atmosph\u00e8re (a\u00e9rosols et mol\u00e9cules de gaz).<\/p>\n\n\n\n<p>Au cours des prochaines d\u00e9cennies, les grands t\u00e9lescopes \u00e9tendront l&#8217;observation \u00e0 de nouveaux domaines spectraux et stimuleront la recherche de vie sur les exoplan\u00e8tes. De nouveaux instruments con\u00e7us pour analyser la composition chimique de la basse atmosph\u00e8re terrestre (gaz \u00e0 effet de serre, polluants, etc.) utilisent des technologies qui permettent de mesurer des spectres avec une tr\u00e8s haute r\u00e9solution spectrale et un rapport signal\/bruit \u00e9lev\u00e9. L&#8217;interpr\u00e9tation de ces spectres n\u00e9cessite la ma\u00eetrise des techniques th\u00e9oriques et exp\u00e9rimentales d&#8217;analyse spectroscopique.<\/p>\n<\/details>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Bibliographie<\/summary>\n<ul class=\"wp-block-list\">\n<li>J.M. Flaud (1992),&nbsp;<em>Spectroscopie des mol\u00e9cules d\u2019int\u00e9r\u00eat atmosph\u00e9rique<\/em>, Ecole d\u2019\u00e9t\u00e9 du CNRS.<\/li>\n\n\n\n<li>J.M. Hollas (2003),&nbsp;<em>Spectroscopie<\/em>, Dunod, 400 pp.<\/li>\n\n\n\n<li>J.M. Hollas (2004),&nbsp;<em>Modern spectroscopy<\/em>, John Wiley &amp; Sons, Inc., 482 pp.<\/li>\n\n\n\n<li>S. Payan (2013),&nbsp;<em>Radiative transfer and inversion<\/em>, Ecole d\u2019\u00e9t\u00e9 du CNRS &#8220;HiResMIR@CAES-Frejus-2013&#8221;, Fr\u00e9jus (France), 3-7 June 2013.<\/li>\n\n\n\n<li>L. R\u00e9galia, H. Tran, M. Leperec (2015),&nbsp;<em>SpecAtmo summer school trainings<\/em>, Fr\u00e9jus (France).<\/li>\n\n\n\n<li>J. Vander Auwera (2013),&nbsp;<em>Principles of vibration-rotation spectroscopy<\/em>, Ecole d\u2019\u00e9t\u00e9 du CNRS &#8220;HiResMIR@CAES-Frejus-2013&#8221;, Fr\u00e9jus (France), 3-7 June 2013.<\/li>\n<\/ul>\n<\/details>\n\n\n\n<h4 class=\"wp-block-heading\">Introduction au transfert radiatif<\/h4>\n\n\n\n<p>Professeur : Cyril Crevoisier<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Aper\u00e7u<\/summary>\n<p>Ce cours pr\u00e9sente les concepts de transfert radiatif direct et inverse, qui sous-tendent l&#8217;\u00e9tude de l&#8217;atmosph\u00e8re terrestre \u00e0 l&#8217;aide de satellites de t\u00e9l\u00e9d\u00e9tection, dans le contexte des \u00e9tudes climatiques. Les variables physiques et les lois fondamentales sont rappel\u00e9es, ce qui conduit \u00e0 la d\u00e9rivation de l&#8217;\u00e9quation de transfert radiatif qui calcule le rayonnement \u00e9lectromagn\u00e9tique transmis ou \u00e9mis par l&#8217;atmosph\u00e8re et mesur\u00e9 \u00e0 sa surface. Cette \u00e9quation implique diverses informations thermodynamiques, spectroscopiques et instrumentales. Les principaux codes de transfert radiatif sont d\u00e9crits. Enfin, le probl\u00e8me inverse qui consiste \u00e0 extraire les variables atmosph\u00e9riques \u00e0 partir de mesures radiom\u00e9triques est abord\u00e9 et illustr\u00e9 par de nombreux exemples impliquant des missions spatiales actuelles.<\/p>\n<\/details>\n<\/details>\n<\/div>\n\n\n\n<div class=\"wp-block-column has-background is-layout-flow wp-block-column-is-layout-flow\" style=\"background-color:#00690014;padding-top:var(--wp--preset--spacing--30);padding-right:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--30);padding-left:var(--wp--preset--spacing--30)\">\n<h3 class=\"wp-block-heading\">Radiom\u00e9trie et t\u00e9l\u00e9d\u00e9tection active  1 &#8211; 6 ECTS<\/h3>\n\n\n\n<p>Responsable : St\u00e9phane Jacquemoud<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>En savoir plus<\/summary>\n<h4 class=\"wp-block-heading\">Th\u00e9orie des antennes<\/h4>\n\n\n\n<p>Professeur : Benoit Poussot <\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Aper\u00e7u<\/summary>\n<ul class=\"wp-block-list\">\n<li>Principe de rayonnement d\u2019une antenne<\/li>\n\n\n\n<li>Description des diff\u00e9rents types d\u2019antennes et de leur utilisation<\/li>\n\n\n\n<li>Caract\u00e9ristiques des antennes<\/li>\n\n\n\n<li>Rayonnement des courants<\/li>\n\n\n\n<li>Rayonnement des ouvertures planes<\/li>\n\n\n\n<li>Bilan de liaison<\/li>\n\n\n\n<li>R\u00e9seaux d\u2019antennes et syst\u00e8mes multi antennes<\/li>\n\n\n\n<li>Principe de radiom\u00e9trie<\/li>\n\n\n\n<li>Qualit\u00e9s radiom\u00e9triques d\u2019une antenne<\/li>\n<\/ul>\n<\/details>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Bibliographie<\/summary>\n<p>Picon O. (2009),&nbsp;<em>Les Antennes : th\u00e9orie, conception et applications<\/em>, Dunod, 371 pp.<\/p>\n<\/details>\n\n\n\n<h4 class=\"wp-block-heading\">T\u00e9l\u00e9d\u00e9tection LiDAR<\/h4>\n\n\n\n<p>Professeur : Fran\u00e7ois Ravetta<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Aper\u00e7u<\/summary>\n<p><\/p>\n<\/details>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Bibliographie<\/summary>\n<p><\/p>\n<\/details>\n\n\n\n<h4 class=\"wp-block-heading\">T\u00e9l\u00e9d\u00e9tection micro-ondes<\/h4>\n\n\n\n<p>Professeur : Alice Le Gall<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Aper\u00e7u<\/summary>\n<p>Ce cours est une introduction aux techniques d&#8217;observation de la Terre par micro-ondes passives et actives.<\/p>\n<\/details>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Bibliographie<\/summary>\n<ul class=\"wp-block-list\">\n<li>Le Chevalier F. (2000),&nbsp;<em>Principes de traitement des signaux Radar et Sonar<\/em>, Masson, 270 pp.<\/li>\n\n\n\n<li>Ulaby F.T., Moore R.K., Fung A.K. (1986),&nbsp;<em>Microwave Remote Sensing: Active and Passive, Volume I: Fundamentals and<\/em> <em>Radiometry<\/em>, Artech House Publishers, 456 pp.<\/li>\n\n\n\n<li>Ulaby F.T., Moore R.K., Fung A.K. (1986),&nbsp;<em>Microwave Remote Sensing: Active and Passive, Volume II: Radar Remote Sensing<\/em> <em>and Surface Scattering and Emission Theory<\/em>, Artech House Publishers, 608 pp.<\/li>\n\n\n\n<li>Ulaby F.T., Moore R.K., Fung A.K. (1986),&nbsp;<em>Microwave Remote Sensing: Active and Passive, Volume III: From Theory to<\/em> <em>Applications<\/em>, Artech House Publishers, 1120 pp.<\/li>\n<\/ul>\n<\/details>\n\n\n\n<h4 class=\"wp-block-heading\">Satellite Imaging Systems<\/h4>\n\n\n\n<p>Professeur : Camille Desjardins<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Aper\u00e7u<\/summary>\n<p>Aper\u00e7u des syst\u00e8mes d&#8217;imagerie par satellite d&#8217;observation de la Terre dans le domaine r\u00e9flectif.<\/p>\n<\/details>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Bibliographie<\/summary>\n<p>Lier P., Valorge C., Briottet X. (2008),&nbsp;<em>Imagerie spatiale : des principes d&#8217;acquisition au traitement des images optiques pour<\/em> <em>l&#8217;observation de la Terre<\/em>, Cepadues Editions, 844 pp.<\/p>\n<\/details>\n\n\n\n<h4 class=\"wp-block-heading\">T\u00e9l\u00e9d\u00e9tection atmosph\u00e9rique<\/h4>\n\n\n\n<p>Professeur : Benoit Laurent<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Aper\u00e7u<\/summary>\n<p>Cette conf\u00e9rence vise \u00e0 donner un aper\u00e7u g\u00e9n\u00e9ral des questions scientifiques li\u00e9es aux probl\u00e8mes soci\u00e9taux tels que le changement climatique, la pollution, etc., ainsi que des outils d&#8217;observation spatiale utilis\u00e9s pour surveiller, analyser et comprendre ces probl\u00e8mes.<\/p>\n<\/details>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Bibliographie<\/summary>\n<ul class=\"wp-block-list\">\n<li>Boucher O. (2012),&nbsp;<em>A\u00e9rosols atmosph\u00e9riques<\/em><strong><em>&nbsp;&#8211;<\/em><\/strong><em>&nbsp;Propri\u00e9t\u00e9s et impacts climatiques<\/em>, Collection : Ing\u00e9nierie et d\u00e9veloppement durable, XIV, Springer, 248 pp.<\/li>\n\n\n\n<li>Burrows J.P., Platt U., Borrell P. (2011),&nbsp;<em>The remote sensing of tropospheric composition from space<\/em>, Physics of Earth and Space Environments, XXXII, Springer, 549 pp.<\/li>\n\n\n\n<li>Lee K.H., Li Z., Kim Y.J., Kokhanovsky A. (2009), Atmospheric aerosol monitoring from satellite observations: A history of three decades, in&nbsp;<em>Atmospheric and biological environmental monitoring<\/em>, Springer, pp 13-38.<\/li>\n<\/ul>\n<\/details>\n\n\n\n<h4 class=\"wp-block-heading\">T\u00e9l\u00e9d\u00e9tection des surfaces terrestres<\/h4>\n\n\n\n<p>Professeur : St\u00e9phane Jacquemoud<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Aper\u00e7u<\/summary>\n<p>Cette conf\u00e9rence est une introduction \u00e0 la caract\u00e9risation des surfaces terrestres par t\u00e9l\u00e9d\u00e9tection, principalement dans le domaine solaire. Dans un premier temps, les diff\u00e9rents modes d&#8217;interaction du rayonnement solaire avec les surfaces continentales sont abord\u00e9s. La deuxi\u00e8me partie du cours est consacr\u00e9e \u00e0 la d\u00e9termination des param\u00e8tres biochimiques et structurels de la v\u00e9g\u00e9tation par t\u00e9l\u00e9d\u00e9tection hyperspectrale et multiangulaire, de l&#8217;\u00e9chelle de la feuille \u00e0 celle de l&#8217;\u00e9cosyst\u00e8me. Dans la derni\u00e8re partie, nous abordons la quantification du bilan \u00e9nerg\u00e9tique \u00e0 la surface de la Terre et son importance dans les mod\u00e8les climatiques. L&#8217;accent est mis sur la mod\u00e9lisation physique \u00e0 diff\u00e9rentes \u00e9chelles.<\/p>\n<\/details>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Bibliographie<\/summary>\n<ul class=\"wp-block-list\">\n<li>Asrar G. (1989),&nbsp;<em>Theory and applications of optical remote sensing<\/em>, Wiley Interscience, 734 pp.<\/li>\n\n\n\n<li>Berthier S. (1993),&nbsp;<em>Optique des milieux composites<\/em>, Polytechnica, 300 pp.<\/li>\n\n\n\n<li>Campbell G.S., Norman J.M. (1998),&nbsp;<em>An introduction to environmental biophysics<\/em>, Springer, 286 pp.<\/li>\n\n\n\n<li>Elias M., Lafait J. (2006),&nbsp;<em>La couleur. Lumi\u00e8re, vision et mat\u00e9riaux<\/em>, Belin, 352 pp.<\/li>\n\n\n\n<li>Gates D.M. (2003),&nbsp;<em>Biophysical ecology<\/em>, Dover, 611 pp.<\/li>\n\n\n\n<li>Hapke B. (1993),&nbsp;<em>Theory of reflectance and emittance spectroscopy<\/em>, Cambridge University Press, 455 pp.<\/li>\n\n\n\n<li>Hufty A. (2001),&nbsp;<em>Introduction \u00e0 la climatologie<\/em>, De Boeck-Universit\u00e9, 542 pp.<\/li>\n\n\n\n<li>Jones H.G., Vaughan R.A. (2010),&nbsp;<em>Remote sensing of vegetation: principles, techniques, and applications<\/em>, Oxford University Press, 353 pp.<\/li>\n\n\n\n<li>Liang S. (2003),&nbsp;<em>Quantitative remote sensing of land surfaces<\/em>, Wiley-Interscience, 560 pp.<\/li>\n\n\n\n<li>Monteith J.L., Unsworth M.H. (2008),&nbsp;<em>Principles of environmental physics<\/em>, Academic Press, 418 pp.<\/li>\n\n\n\n<li>Myneni R.B., Ross J. (1991),&nbsp;<em>Photon-vegetation interactions: applications in optical remote sensing and plant ecology<\/em>, Springer-Verlag, 565 pp.<\/li>\n<\/ul>\n<\/details>\n<\/details>\n<\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-28f84493 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column has-background is-layout-flow wp-block-column-is-layout-flow\" style=\"background-color:#00690014;padding-top:var(--wp--preset--spacing--30);padding-right:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--30);padding-left:var(--wp--preset--spacing--30)\">\n<h3 class=\"wp-block-heading\">Radiom\u00e9trie et t\u00e9l\u00e9d\u00e9tection active 2<\/h3>\n\n\n\n<p>Responsable : <\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>En savoir plus<\/summary>\n<p><\/p>\n<\/details>\n<\/div>\n\n\n\n<div class=\"wp-block-column has-background is-layout-flow wp-block-column-is-layout-flow\" style=\"background-color:#00690014;padding-top:var(--wp--preset--spacing--30);padding-right:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--30);padding-left:var(--wp--preset--spacing--30)\">\n<h3 class=\"wp-block-heading\">Orbites satellitaires et g\u00e9od\u00e9sie &#8211; 3 ECTS<\/h3>\n\n\n\n<p>Responsable : Florent Deleflie<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>En savoir plus<\/summary>\n<p>Le cours propose l\u2019acquisition des notions fondamentales \u00e0 l\u2019\u00e9tude des trajectoires de satellites artificiels autour de la Terre. Il permet de revoir les lois de Kepler et leurs applications, permet d\u2019\u00e9tudier les principales perturbations qui font s\u2019\u00e9carter le mouvement r\u00e9el du mouvement k\u00e9pl\u00e9rien.<\/p>\n\n\n\n<p>Les applications concernent \u00e0 la fois la description des principales familes dynamiques, en r\u00e9gion LEO (les orbites basses), en r\u00e9gion MEO (les orbites moyennes), et la r\u00e9gion GSO (les g\u00e9osynchrones), en metant l\u2019accent sur la famille des h\u00e9liosyncrhones, les SSO, si impotante pour l\u2019observation de la Terre et la t\u00e9l\u00e9d\u00e9tection.<br>Les s\u00e9ances de cours font alterner cours magistraux, s\u00e9an ces d\u2019exercices et trav aux sur ordinateur.<br>Les enjeux li\u00e9s \u00e0 l\u2019environnement spatial de la Terre sont aussi pr\u00e9sent\u00e9s.<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Bibliographie<\/summary>\n<p><\/p>\n<\/details>\n<\/details>\n<\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-28f84493 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column has-background is-layout-flow wp-block-column-is-layout-flow\" style=\"background-color:#00690014;padding-top:var(--wp--preset--spacing--30);padding-right:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--30);padding-left:var(--wp--preset--spacing--30)\">\n<h3 class=\"wp-block-heading\">Data science &#8211; Basique<\/h3>\n\n\n\n<p>Responsable : Ga\u00eblle de Coetlogon<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>En savoir plus<\/summary>\n<h4 class=\"wp-block-heading\">Traitement du signal<\/h4>\n\n\n\n<p>Professeur : Ga\u00eblle de Coetlogon<br>Organisation :<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Aper\u00e7u<\/summary>\n<p><\/p>\n<\/details>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Bibliographie<\/summary>\n<p><\/p>\n<\/details>\n\n\n\n<h4 class=\"wp-block-heading\">Analyse de donn\u00e9es<\/h4>\n\n\n\n<p>Professeur : Ga\u00eblle de Coetlogon<br>Organisation :<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Aper\u00e7u<\/summary>\n<p><\/p>\n<\/details>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>Bibliographie<\/summary>\n<p><\/p>\n<\/details>\n<\/details>\n<\/div>\n\n\n\n<div class=\"wp-block-column has-background is-layout-flow wp-block-column-is-layout-flow\" style=\"background-color:#00690014;padding-top:var(--wp--preset--spacing--30);padding-right:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--30);padding-left:var(--wp--preset--spacing--30)\">\n<h3 class=\"wp-block-heading\">Data science &#8211; avanc\u00e9 &#8211; 3 ECTS<\/h3>\n\n\n\n<p>Responsable : Nobuaki Fuji<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>En savoir plus<\/summary>\n<p>Equipe p\u00e9dagogique : Nobuaki Fuji, Guillaume Gastineau, C. Mejia, H\u00e9l\u00e8ne Chepfer, S\u00e9bastien Rodriguez<\/p>\n\n\n\n<p>Dans ce cours, nous enseignerons trois mati\u00e8res diff\u00e9rentes : la th\u00e9orie des probl\u00e8mes inverses (N. Fuji), les r\u00e9seaux neuronaux et l&#8217;IA (G. Gastineau, C. Mejia) et PW en science des donn\u00e9es avanc\u00e9e (ESA, H. Chepfer, S. Rodriguez). Nous pr\u00e9senterons une introduction g\u00e9n\u00e9rale \u00e0 la th\u00e9orie des probl\u00e8mes inverses et explorerons quelques exemples concrets, en utilisant des techniques de pointe telles que l&#8217;intelligence artificielle. Le cours sera dispens\u00e9 en fran\u00e7ais, ou en anglais s&#8217;il y a des \u00e9tudiants non francophones.<\/p>\n<\/details>\n<\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-28f84493 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column has-background is-layout-flow wp-block-column-is-layout-flow\" style=\"background-color:#00690014;padding-top:var(--wp--preset--spacing--30);padding-right:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--30);padding-left:var(--wp--preset--spacing--30)\">\n<h3 class=\"wp-block-heading\">Mod\u00e9lisation pour la t\u00e9l\u00e9d\u00e9tection &#8211; 3 ECTS<\/h3>\n\n\n\n<p>Responsable : <\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>En savoir plus<\/summary>\n<p><\/p>\n<\/details>\n<\/div>\n\n\n\n<div class=\"wp-block-column has-background is-layout-flow wp-block-column-is-layout-flow\" style=\"background-color:#00690014;padding-top:var(--wp--preset--spacing--30);padding-right:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--30);padding-left:var(--wp--preset--spacing--30)\">\n<h3 class=\"wp-block-heading\">Orbites satellitaires &#8211; 3 ECTS<\/h3>\n\n\n\n<p>Responsable :<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>En savoir plus<\/summary>\n<p><\/p>\n<\/details>\n<\/div>\n<\/div>\n<\/div>\n\n\n\n<div id=\"M2\" class=\"wp-block-group is-layout-constrained wp-block-group-is-layout-constrained\">\n<h2 class=\"wp-block-heading\">UE optionnelles disponibles (2 au choix)<\/h2>\n\n\n\n<div style=\"height:50px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-28f84493 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column has-background is-layout-flow wp-block-column-is-layout-flow\" style=\"background-color:#00690014;padding-top:var(--wp--preset--spacing--30);padding-right:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--30);padding-left:var(--wp--preset--spacing--30)\">\n<h3 class=\"wp-block-heading\"><strong>Chimie atmosph\u00e9rique et qualit\u00e9 de l&#8217;air<\/strong> &#8211; 3 ECTS<\/h3>\n\n\n\n<p>\u00c9quipe p\u00e9dagogique : Sol\u00e8ne Turquety*<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>En savoir plus<\/summary>\n<p>Ce cours vise \u00e0 pr\u00e9senter les m\u00e9canismes chimiques et physiques qui r\u00e9gissent l&#8217;\u00e9quilibre des composants \u00e0 courte dur\u00e9e de vie de l&#8217;atmosph\u00e8re, les gaz \u00e0 l&#8217;\u00e9tat de traces et les a\u00e9rosols. Comprendre et suivre leur \u00e9volution dans l&#8217;atmosph\u00e8re est un enjeu soci\u00e9tal majeur, compte tenu de leur r\u00f4le cl\u00e9 dans l&#8217;habitabilit\u00e9 de la plan\u00e8te et des impacts forts d&#8217;un d\u00e9s\u00e9quilibre : d\u00e9gradation de la couche d&#8217;ozone dans la stratosph\u00e8re, d\u00e9gradation de la qualit\u00e9 de l&#8217;air pr\u00e8s de la surface, nombreuses interactions avec le climat. Les m\u00e9canismes impliqu\u00e9s seront d\u00e9crits par une combinaison d&#8217;expos\u00e9s, d&#8217;exercices appliqu\u00e9s et de travaux pratiques num\u00e9riques.<\/p>\n\n\n\n<p>Une premi\u00e8re partie introduit les bases de la cin\u00e9tique chimique et des \u00e9quilibres photochimiques dans la troposph\u00e8re. L&#8217;\u00e9quilibre de la stratosph\u00e8re et d&#8217;\u00e9volution de la couche d&#8217;ozone sont ensuite \u00e9tudi\u00e9s. Le reste du cours est consacr\u00e9 plus sp\u00e9cifiquement \u00e0 la compr\u00e9hension de la capacit\u00e9 oxydante de la troposph\u00e8re et de la composition et des propri\u00e9t\u00e9s des a\u00e9rosols atmosph\u00e9riques. Les principaux processus impliqu\u00e9s dans le d\u00e9veloppement des \u00e9pisodes de pollution atmosph\u00e9rique \u00e0 l&#8217;\u00e9chelle urbaine et r\u00e9gionale, ainsi que les outils utilis\u00e9s par la communaut\u00e9 scientifique et les services de gestion de la qualit\u00e9 de l&#8217;air pour la surveillance et la pr\u00e9vision de la qualit\u00e9 de l&#8217;air, sont ensuite d\u00e9crits. Enfin, les nombreuses interactions entre chimie r\u00e9active et climat sont introduites.&nbsp;<\/p>\n<\/details>\n<\/div>\n\n\n\n<div class=\"wp-block-column has-background is-layout-flow wp-block-column-is-layout-flow\" style=\"background-color:#00690014;padding-top:var(--wp--preset--spacing--30);padding-right:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--30);padding-left:var(--wp--preset--spacing--30)\">\n<h3 class=\"wp-block-heading\">Nuages, a\u00e9rosols et pr\u00e9cipitations &#8211; 3 ECTS<\/h3>\n\n\n\n<p>\u00c9quipe p\u00e9dagogique : H\u00e9l\u00e8ne Chepfer, Jean-Christophe Raut <\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>En savoir plus<\/summary>\n<p>Les nuages constituent la partie visible du cycle de l&#8217;eau dans l&#8217;atmosph\u00e8re. Ils r\u00e9gulent les pr\u00e9cipitations et la vapeur d&#8217;eau atmosph\u00e9rique, interagissent avec la surface et la pollution (par exemple en produisant du smog) et sont l&#8217;un des principaux modulateurs de la temp\u00e9rature terrestre gr\u00e2ce \u00e0 leur interaction avec les rayonnements solaires et telluriques. Les particules d&#8217;a\u00e9rosol jouent un r\u00f4le important sur la qualit\u00e9 de l&#8217;air, mais aussi sur le climat par leur interaction avec le rayonnement et les nuages. Sans particules d&#8217;a\u00e9rosol, la formation de nuages dans l&#8217;atmosph\u00e8re ne se produirait pas aux temp\u00e9ratures et aux humidit\u00e9s relatives auxquelles on observe l&#8217;existence de nuages.<\/p>\n\n\n\n<p>Ce cours pr\u00e9sente les \u00e9l\u00e9ments cl\u00e9s de la physique des a\u00e9rosols, des nuages et des pr\u00e9cipitations, depuis l&#8217;\u00e9chelle locale (les particules composant les nuages) jusqu&#8217;\u00e0 l&#8217;\u00e9chelle r\u00e9gionale (un syst\u00e8me nuageux) et \u00e0 l&#8217;\u00e9chelle mondiale.<\/p>\n\n\n\n<p>Il comprend :<br>&#8211; R\u00e9troactions des nuages et lien avec la sensibilit\u00e9 climatique.<br>&#8211; Origine et composition chimique des a\u00e9rosols<br>&#8211; R\u00e9partition spatiale et verticale des particules dans l&#8217;atmosph\u00e8re<br>&#8211; Microphysique des a\u00e9rosols : mouvement brownien, coagulation, condensation, d\u00e9p\u00f4t, nucl\u00e9ation des nuages<br>&#8211; Propri\u00e9t\u00e9s optiques des a\u00e9rosols<br>&#8211; For\u00e7age radiatif des a\u00e9rosols : direct, semi-direct, indirect, impact sur les surfaces enneig\u00e9es et glac\u00e9es<br>&#8211; L&#8217;eau dans l&#8217;atmosph\u00e8re : thermodynamique de l&#8217;air humide<br>&#8211; Microphysique des nuages chauds : formation et croissance des gouttelettes nuageuses<br>&#8211; Microphysique des nuages froids : formation et croissance des cristaux de glace<br>&#8211; Processus de pr\u00e9cipitation : pluie et neige<br>&#8211; Propri\u00e9t\u00e9s optiques des nuages<br>&#8211; Effet des nuages sur les rayonnements<\/p>\n<\/details>\n<\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-28f84493 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column has-background is-layout-flow wp-block-column-is-layout-flow\" style=\"background-color:#00690014;padding-top:var(--wp--preset--spacing--30);padding-right:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--30);padding-left:var(--wp--preset--spacing--30)\">\n<h3 class=\"wp-block-heading\">\u00c9nerg\u00e9tique du syst\u00e8me climatique<\/h3>\n\n\n\n<p>\u00c9quipe p\u00e9dagogique : <\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>En savoir plus<\/summary>\n<p>Professeurs : <br>Organisation : <\/p>\n<\/details>\n<\/div>\n\n\n\n<div class=\"wp-block-column has-background is-layout-flow wp-block-column-is-layout-flow\" style=\"background-color:#00690014;padding-top:var(--wp--preset--spacing--30);padding-right:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--30);padding-left:var(--wp--preset--spacing--30)\">\n<h3 class=\"wp-block-heading\">Masterclass : Acad\u00e9mie spatiale<\/h3>\n\n\n\n<p>\u00c9quipe p\u00e9dagogique : Philippe Lognonn\u00e9*, Delphine Urbah, et intervenants invit\u00e9s<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>En savoir plus<\/summary>\n<p>The MasterClass, hosted by the Acad\u00e9mie Spatiale d\u2019Ile de France and Universit\u00e9 Paris Cit\u00e9, take place during a full week in February.&nbsp; It is open to all students of Space related masters from all Universities of Ile de France.<\/p>\n\n\n\n<p>The 2025 and 2026 editions will be focused on &#8220;&#8221;Earth Resources Remote Sensing and Extra-terrestrial Resources Exploration and Utilization,&#8221;<\/p>\n\n\n\n<p>During this week, 18 lectures will present the cutting-edge technologies in Earth resource monitoring from space, water related geodesy, and Earth remote sensing, as well as the exploration and utilization of extraterrestrial resources.&nbsp;<\/p>\n\n\n\n<p>Lecturers are from leading research laboratories (Polytechnique Montreal, CESBIO, GFZ Postam, Universit\u00e9 Luxembourg, Universit\u00e9 Paris Saclay, Institut de physique du Globe de Paris), large and small companies (Total Energy, Blue Origin, Ispace, MinersAI) and space agencies and international organizations (ESA, EEC, CNES).&nbsp;<\/p>\n\n\n\n<p>In addition to space related technologies, both in terms of instrumentation, data acquisition, data analysis and interpretation, some lectures present also AI applications, policy frameworks, and space mining economy.&nbsp;<\/p>\n\n\n\n<p>In addition to the 18 lectures, the program will offer one site visits, and case studies to provide hands-on experience. Lunches with the lecturers and a social event during one of the evening will offer networking opportunities and interactions with scientists and ingeneers involved in space utilization and space exploration. Two of the lectures are Directed Works.<\/p>\n\n\n\n<p>The evaluation is made through a QCM sent to the students a few weeks after the MasterClass and which has to be returned within 72 hours.<\/p>\n<\/details>\n<\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-28f84493 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column has-background is-layout-flow wp-block-column-is-layout-flow\" style=\"background-color:#00690014;padding-top:var(--wp--preset--spacing--30);padding-right:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--30);padding-left:var(--wp--preset--spacing--30)\">\n<h3 class=\"wp-block-heading\"><strong>T\u00e9l\u00e9d\u00e9tection des d\u00e9formations tectoniques et volcaniques<\/strong><\/h3>\n\n\n\n<p>\u00c9quipe p\u00e9dagogique : Rapha\u00ebl Grandin*, Jean-Mathieu Nocquet, Arthur Delorme<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>En savoir plus<\/summary>\n<ul class=\"wp-block-list\">\n<li>General introduction to space geodesy (3h course) : shape of the Earth, gravity field, geoid, satellite orbits, geodetic techniques.<\/li>\n\n\n\n<li>InSAR (3h course + 3h practical) : radar image formation, satellite acquisition modes, interferometry, atmospheric artifacts, applications to volcanic and tectonic deformation, processing of a real dataset.<\/li>\n\n\n\n<li>GNSS (3h course + 3h practical) : basic principles, ionospheric and atmospheric corrections, reference frame, applications to seismic cycle, application to a real dataset.<\/li>\n\n\n\n<li>Optical imagery (1h course + 2h practical) : optical image geometry, bundle adjustment, stereophotogrammetry, sub-pixel correlation, application to a real dataset.<\/li>\n\n\n\n<li>Modeling (1h course + 2h practical) : basic principles of inverse problem theory, seismic slip inversion, volcano deformation, application to a real dataset.<\/li>\n<\/ul>\n<\/details>\n<\/div>\n\n\n\n<div class=\"wp-block-column has-background is-layout-flow wp-block-column-is-layout-flow\" style=\"background-color:#00690014;padding-top:var(--wp--preset--spacing--30);padding-right:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--30);padding-left:var(--wp--preset--spacing--30)\">\n<h3 class=\"wp-block-heading\"><strong>T\u00e9l\u00e9d\u00e9tection de l&#8217;hydrosph\u00e8re et de la cryosph\u00e8re<\/strong><\/h3>\n\n\n\n<p>\u00c9quipe p\u00e9dagogique : Olivier Bock*, Laurent Metivier, Manon Dalaison<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>En savoir plus<\/summary>\n<p>This course introduces the fundamentals of the Earth\u2019s water cycle, with a special focus on the hydrosphere and cryosphere, and their observation using remote sensing techniques, particularly geodesy and gravimetry methods.<\/p>\n\n\n\n<p>The course is organized around general lectures and practical sessions covering the following topics:<\/p>\n\n\n\n<ul class=\"wp-block-list\">\n<li>The Earth\u2019s water cycle: stores, fluxes, and their quantification<\/li>\n\n\n\n<li>Remote sensing of atmospheric water vapor using GNSS<\/li>\n\n\n\n<li>Remote sensing of the hydrosphere and cryosphere with geodesy and gravimetry<\/li>\n\n\n\n<li>Monitoring surface and underground water resources<\/li>\n\n\n\n<li>Past and recent changes in global ice mass budget, sea level height, and atmospheric water vapor<\/li>\n<\/ul>\n\n\n\n<p>The course includes an individual research project, which can involve:<\/p>\n\n\n\n<ul class=\"wp-block-list\">\n<li>A study of a scientific paper<\/li>\n\n\n\n<li>Thematic data analysis<\/li>\n\n\n\n<li>The development or testing of a remote sensing algorithm<\/li>\n<\/ul>\n<\/details>\n<\/div>\n<\/div>\n\n\n\n<div class=\"wp-block-columns is-layout-flex wp-container-core-columns-is-layout-28f84493 wp-block-columns-is-layout-flex\">\n<div class=\"wp-block-column has-background is-layout-flow wp-block-column-is-layout-flow\" style=\"background-color:#00690014;padding-top:var(--wp--preset--spacing--30);padding-right:var(--wp--preset--spacing--30);padding-bottom:var(--wp--preset--spacing--30);padding-left:var(--wp--preset--spacing--30)\">\n<h3 class=\"wp-block-heading\"><strong>T\u00e9l\u00e9d\u00e9tection des surfaces plan\u00e9taires<\/strong><\/h3>\n\n\n\n<p>\u00c9quipe p\u00e9dagogique : C\u00e9cile Ferrari*, S\u00e9bastien Rodriguez<\/p>\n\n\n\n<details class=\"wp-block-details is-layout-flow wp-block-details-is-layout-flow\"><summary>En savoir plus<\/summary>\n<ul class=\"wp-block-list\">\n<li>The Golden Age of Solar System exploration: from light dots to new worlds. An history of space exploration. General questions on the origin and evolution of the Solar System. Surfaces scars as fingerprints of endogenic and exogenic evolution processes: bombardments, space weathering, topography, composition.<\/li>\n\n\n\n<li>Multi-wavelengths remote sensing strategy: from radio to gamma photons. How to probe surfaces at various depths. Imaging and spectroscopy. Light-matter interactions and remote sensing instruments. Examples.<\/li>\n\n\n\n<li>From observations to structure and composition: modelling planetary surfaces. Commonly used analytical models. Modeling particles and surface scattering, energy balance and thermal emission.<\/li>\n\n\n\n<li>Methodology (after Python lectures, end of semester) with Python 3 and Notebooks: Photometric models of planetary surfaces, energy balance and radiometry, thermal emission<\/li>\n<\/ul>\n<\/details>\n<\/div>\n\n\n\n<div class=\"wp-block-column is-layout-flow wp-block-column-is-layout-flow\"><\/div>\n<\/div>\n<\/div>\n","protected":false},"excerpt":{"rendered":"<p>Tronc commun &#8211; 54 ECTS Rayonnement \u00e9lectromagn\u00e9tique &#8211; 3 ECTS Responsable UE : Shermila Mostarshedi Stages et s\u00e9minaires &#8211; 3 [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"site-sidebar-layout":"default","site-content-layout":"","ast-site-content-layout":"default","site-content-style":"default","site-sidebar-style":"default","ast-global-header-display":"","ast-banner-title-visibility":"","ast-main-header-display":"","ast-hfb-above-header-display":"","ast-hfb-below-header-display":"","ast-hfb-mobile-header-display":"","site-post-title":"","ast-breadcrumbs-content":"","ast-featured-img":"","footer-sml-layout":"","ast-disable-related-posts":"","theme-transparent-header-meta":"","adv-header-id-meta":"","stick-header-meta":"","header-above-stick-meta":"","header-main-stick-meta":"","header-below-stick-meta":"","astra-migrate-meta-layouts":"default","ast-page-background-enabled":"default","ast-page-background-meta":{"desktop":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"tablet":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"mobile":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""}},"ast-content-background-meta":{"desktop":{"background-color":"var(--ast-global-color-4)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"tablet":{"background-color":"var(--ast-global-color-4)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"mobile":{"background-color":"var(--ast-global-color-4)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""}},"footnotes":""},"class_list":["post-578","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/paris-remote-sensing-master.fr\/index.php?rest_route=\/wp\/v2\/pages\/578","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/paris-remote-sensing-master.fr\/index.php?rest_route=\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/paris-remote-sensing-master.fr\/index.php?rest_route=\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/paris-remote-sensing-master.fr\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/paris-remote-sensing-master.fr\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=578"}],"version-history":[{"count":85,"href":"https:\/\/paris-remote-sensing-master.fr\/index.php?rest_route=\/wp\/v2\/pages\/578\/revisions"}],"predecessor-version":[{"id":1004,"href":"https:\/\/paris-remote-sensing-master.fr\/index.php?rest_route=\/wp\/v2\/pages\/578\/revisions\/1004"}],"wp:attachment":[{"href":"https:\/\/paris-remote-sensing-master.fr\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=578"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}