The LHCb experiment is dedicated to precision measurements of CP violation and rare decays of B hadrons at the Large Hadron Collider (LHC) at CERN (Geneva). The initial configuration and expected performance of the detector and associated systems, as established by test beam measurements and simulation studies, is described.

NA62 is a fixed-target experiment at the CERN SPS dedicated to measurements of rare kaon decays. Such measurements, like the branching fraction of the K+ → π+ ν ν̄ decay, have the potential to bring significant insights into new physics processes when comparison is made with precise theoretical predictions. For this purpose, innovative techniques have been developed, in particular, in the domain of low-mass tracking devices. Detector construction spanned several years from 2009 to 2014. The collaboration started detector commissioning in 2014 and will collect data until the end of 2018. The beam line and detector components are described together with their early performance obtained from 2014 and 2015 data.

region at a hadron collider. This document discusses the implications of these first measurements on classes of extensions to the Standard Model, bearing in mind the interplay with the results of searches for on-shell production of new particles at ATLAS and CMS. The physics potential of an upgrade to the LHCb detector, which would allow an order of magnitude more data to be collected, is emphasised.

S U M M A R YPotential fields are classically represented on the sphere using spherical harmonics. However, this decomposition leads to numerical difficulties when data to be modelled are irregularly distributed or cover a regional zone. To overcome this drawback, we develop a new representation of the magnetic and the gravity fields based on wavelet frames.In this paper, we first describe how to build wavelet frames on the sphere. The chosen frames are based on the Poisson multipole wavelets, which are of special interest for geophysical modelling, since their scaling parameter is linked to the multipole depth (Holschneider et al.). The implementation of wavelet frames results from a discretization of the continuous wavelet transform in space and scale. We also build different frames using two kinds of spherical meshes and various scale sequences. We then validate the mathematical method through simple fits of scalar functions on the sphere, named 'scalar models'. Moreover, we propose magnetic and gravity models, referred to as 'vectorial models', taking into account geophysical constraints. We then discuss the representation of the Earth's magnetic and gravity fields from data regularly or irregularly distributed. Comparisons of the obtained wavelet models with the initial spherical harmonic models point out the advantages of wavelet modelling when the used magnetic or gravity data are sparsely distributed or cover just a very local zone.Magnetic and gravity observations are of great importance for the understanding of geodynamic activity of our planet. Measurements of the Earth's magnetic and gravity fields undertaken by satellites (without forgetting those on land, sea and air) are of particular interest, as they provide a global and uniform survey of these fields and of their temporal evolution.Models of the magnetic field have been derived by means of several Earth's satellite missions, which have been carrying magnetic sensors. Satellite-borne magnetometers provide information on strength and direction of the internal and external Earth's magnetic field and its time variations. The Earth is surrounded by a large and complicated field caused to a large extent by a dynamo operating in the fluid core. Currents flowing in the ionosphere, magnetosphere and oceans and magnetized rocks also influenced the geomagnetic field.Three magnetic missions (Ørsted-launched in 1999, CHAMP and SAC-C-launched in 2000) have collected measurements providing new insights into the composition and the processes in the interior, and surrounding of the planet. These observations are also used in a range of applications, including navigation systems, resource exploration drilling, spacecraft attitude control systems and assessments of the impact of space weather. The coming decade will see further missions planned for more in-depth, dedicated studies of magnetic field including DEMETER, 2004; ESPERIA, 2006; Swarm, 2008; etc. Gravity field observations from space can advance our knowledge of the geoid and its time variations. The g...

The Sixth International Comparison of Absolute Gravimeters was held from 5 June to 28 August 2001 at the Bureau International des Poids et Mesures (BIPM), Sèvres. Seventeen absolute gravimeters were used to make measurements at five sites of the BIPM gravity network. The vertical gravity gradients at the sites and the ties between them were also measured using seventeen relative gravimeters. For the first time the ties were also measured using absolute gravimeters. Various methods of processing the absolute and relative data were tested to calculate the results. The final results of ICAG-2001 are presented. The acceleration due to gravity at a height of 0.90 m is given as (980 925 701.2 ± 5.5) µGal* and (980 928 018.8 ± 5.5) µGal for sites A and B, respectively,