Abstract. This review paper is devoted to the presentation of recent progress in the mathematical analysis of equatorial waves. After a short presentation of the physical background, we present some of the main mathematical results related to the problem.More precisely we are interested in the study of the shallow water equations set in the vicinity of the equator: in that situation the Coriolis force vanishes and its linearization near zero leads to the so-called betaplane model. Our aim is to study the asymptotics of this model in the limit of small Rossby and Froude numbers. We show in a first part the existence and uniqueness of bounded (strong) solutions on a uniform time, and we study their weak limit. In a second part we give a more precise account of the asymptotics by characterizing the possible defects of compactness to that limit, in the framework of weak solutions only.These results are based on the studies [6]-[8] on the one hand, and [11] on the other.1. Physical background and goal of the study.1.1. Physical background. The aim of this review paper is to present a mathematical description of oceanic flows in the equatorial zone of the Earth. We are interested in domains extending over many thousands of kilometers, and on such scales the forces with dominating influence are the gravity and the Coriolis force. Our goal is to try to understand how those forces counterbalance each other to impose the so-called geostrophic constraint on the mean motion, and to describe the oscillations which are generated around this geostrophic equilibrium.In this survey we will be concentrating on the equatorial zone. Let us however briefly discuss the situation at midlatitudes, which has been more extensively studied from a mathematical point of view, in the past years. At midlatitudes, on "small" geographical zones (namely for a small enough interval around a given latitude far enough from the equator) one can neglect the variations of the Coriolis force due to the curvature of the Earth, and this leads to a singular perturbation problem with constant coefficients. The corresponding asymptotics (in the limit of a large rotation) have been studied by a number of authors, depending on the boundary conditions, the generality of the initial data... Roughly speaking one may summarize the situation in that case by stating that a limiting behaviour (in the limit of a small Rossby number, meaning that the rotation of the Earth is predominant over the motion under study) can be exhibited, and some sort of convergence (weak or strong depending on the boundaries or on the initial data) can be proved. We refer for instance to the review by R. Temam and M. Ziane [21] or by the author and L. Saint-Raymond [10], or to the work by J.-Y. Chemin, B. Desjardins, the author and E. Grenier [3] for more details.Here we are interested in a geographical zone where the variations of the Coriolis force do play a role (indeed the Coriolis force is identically zero at the equator and has a different sign on each hemisphere); we also wish to...