Ray Tracing Analysis of Light Radiation from Sharp Bends in Graded-Index Multimode Fibers (original) (raw)

Parameters affecting bending losses in graded-index polymer optical fibers

IEEE Journal of Selected Topics in Quantum Electronics, 2001

Radiation losses that occur when bending gradedindex polymer optical fibers (POFs) are analyzed as a function of the profile exponent, the light wavelength, the fiber core radius, and the length of the bent section. For this purpose, a ray-tracing model is used, which combines both the generalized Fresnel power transmission coefficients for curved graded-index media and the differential equations that govern the ray paths in highly multimode graded-index fibers. This model is applied to the most recent types of graded-index POF, for which the choice of the core radius and profile exponent is discussed from the point of view of bending losses (the greater the profile exponent and the core radius, the greater the bending losses). The influence of profile exponents different from two is included for the first time.

An examination of the effect of polarization on the radiation losses of bent optical fibres

Optical and Quantum Electronics, 1993

It has long been recognized that the bending losses in weakly guiding optical fibres are independent of the polarization for large bend radius. Here, we show this fact using the volume equivalent current method. The procedure is then applied to a helically bent fibre and it is shown that the radiation from the helical fibre is also independent of the polarization as long as the fibre is weakly guiding.

Radiation from graded-index single-mode fibres

IEE Proceedings H Microwaves, Optics and Antennas

Radiation from the fundamental mode due to sources in graded-index single-mode optical fibres can be examined by determining the effect of the presence of the perturbing core on the free-space (i.e. uniform cladding) radiation field. We look at this effect for fibres with power-law-profile cores. Using these examples we discuss the following two approximation schemes: (i) a new equivalent step approximation where the step has the same 'degree of guidance' as the graded core and (ii) a previously proposed WKB asymptotic approximation.

Two-dimensional refractive index and stresses profiles of a homogenous bent optical fiber

Applied Optics, 2014

We present a significant contribution to the theory of determining refractive index profile of a bent homogenous optical fibre. In this theory we consider two different processes controlling the index profile variations. The first is the linear index variation, due to stress along the bent radius and the second is the release of this stress on the fibre surface. This release process is considered to be radial dependence on the fibre radius. These considerations enable us to construct the index profile in two dimensions normal to the optical axis, considering the refraction of light rays traversing the fibre. This theory is applied to optical homogenous bent fibre with two bending radii, when they are located orthogonal the light path of the object arm in holographic setup (like Mach-Zehnder interferometer). Digital holographic phase shifting interferometry is employed in this study. The recorded phase shifted holograms have been combined, reconstructed and processed to extract the phase map of the bent optical fibre. A comparison, between the extracted optical phase differences and the calculated one, indicates that the refractive index profile variation should include the above mentioned two processes which are considered as a response for stresses distribution across fiber's cross section. The experimentally obtained refractive indices profiles provide stresses induces birefringence profile. Thus we are able to present realistic induced stresses profile due to bending.

Determination of the width of the output angular power distribution in step-index multimode optical fibers

2010

Two functions for calculating the width of the output angular power distribution are tested for light launched centrally along the axis of a step-index plastic optical fiber. It is found that the more recent of the two agrees better with experimental measurements. The other function (Gloge's) underestimates the output width for longer fiber lengths, which is attributed to it not accounting for an appropriate boundary condition at the critical propagation angle.

Microbending effects on monomode light propagation in multimode fibers

Journal of the Optical Society of America, 1983

The effects of periodic axis deformations on propagation in multimode optical fibers with single-mode excitation are investigated numerically and experimentally. The numerical study, based on ray theory, deals with helical rays in the presence of sinusoidal axis deformations for various shapes of index profile. The corresponding experimental observations and results, carried out on tubular modes, confirm the existence of resonance effects between the helical ray period and the fiber axis deformation. This technique permits the observation of mode-to-mode power transfer and provides a sensitive tool to investigate the mode-coupling mechanism in optical fibers.

Geometric optics analysis of modal propagation in graded-index cylindrical fiber

Applied Optics, 1990

Methods of geometric optics are used to characterize a multimode optical fiber. The discrete propagation modes are derived by applying the phase resonance constraint to equations of constant phase surfaces. This constraint provides a very clear geometrical interpretation of discrete propagation modes, and provides a link between the well known Wentzel, Kramers, Brillouin (WKB) method and geometric optics.

A refractive index in bent fibre optics and curved space

Journal of Physics: Conference Series

The refractive index in the bent fibre optics and in curved space of the gravitational field are studied. We obtain the results that refractive index in the bent fibre optics is similar with refractive index in curved space of the gravitational field. Both results show that refractive index increases when light traverses through the bent fibre optics and curved space of the gravitational field. Based on analogy reasoning taken from fibre optics bending loss phenomena, we propose that if light traverses through curved space of the gravitational field, light will loss its energy. We calculate this energy loss numerically using bending loss model of Faustini-Martini. We find that light losses its energy around 467.7073 dB/m, when it traverses through curved space with radius of curvature R = 0.01 m due to massive object around 8.7 × 10 20 kg.

Numerical Simulation of Radiation from Multimode Optical Fibers

Radiophysics and Quantum Electronics, 2005

We obtain an asymptotic expression for calculation of radiation fields of the waveguide modes of a multimode fiber with a step-like profile of the refractive index at high normalized frequencies. The distribution of intensity of the output radiation is calculated numerically. Statistical characteristics of the calculated speckles are found and compared with the experiment. Rigorous calculation of the intensity distribution of radiation from a multimode optical fiber in the far diffraction region with allowance for the edge effects is a complicated problem [1, 2]. If the number of propagating waveguide modes is large, then application of the classical numerical methods requires long computation time. Therefore, it is difficult or even impossible to implement such methods on a personal computer. For optical fibers (OFs) with step-like profiles of the refractive index, the problem under consideration can be solved analytically using a number of approximations, which reduces the duration of calculations by several orders of magnitude. Correspondingly, new possibilities for studying the parameters of the output radiation by means of numerical simulation appear. Actually, the posed problem consists of two parts, namely, determination of the intensity of the electromagnetic field at the output end of the fiber and calculation of the field in the far diffraction region. The expressions for field intensity of separate waveguide modes are well known. For example, the longitudinal component E z of the electric field can be written as [3, 4] E z (r, ϕ, z) = A ls J l (u ls r/r 0) cos(lϕ + ϕ 0) exp(iβ ls z)/J l (u ls), where l and s are the azimuthal and radial indices of the mode, respectively, A ls is the normalization factor, J l is a Bessel function of the first kind of order l, r 0 is the radius of the OF core, r, ϕ and z are cylindrical coordinates, and u ls and β ls are, respectively, the eigenvalue of the characteristic equation and the axial propagation constant for the mode with indices l and s. For the classical numerical transformation, it is necessary to calculate beforehand the field at the OF output end by summing up the fields of all waveguide modes and, then, to determine the field in the far diffraction region. In the case of analytical solution, it is convenient to calculate at first the field of each waveguide mode in the far zone and, then, to perform summation with allowance for the phase and polarization. Due to the cylindrical symmetry of the initial distribution, it is expedient to use cylindrical coordinates when performing integration in the plane of the OF output end. The concept of calculating the directional pattern and the field intensities by the stationary-phase method is well known [5]. We neglect both the penetration of the fields of the waveguide modes into the fiber cladding and a change in the field as it escapes into free space and assume that cos θ ≈ 1, where θ is the angle of radiation escape. Representing the expression for a plane electromagnetic wave as a sum of Bessel functions [6] and following [5-7], we can reduce the considered problem of radiation escape to the well-known problem of radiation injection [6]. In