# Modes

Definition: self-consistent electric field distributions in waveguides, optical resonators or in free space

More specific terms: guided modes, cladding modes, tunelling modes = leaky modes, resonator modes, Hermite–Gaussian modes, LP modes, higher-order modes

German: Moden

Categories: general optics, fiber optics and waveguides, optical resonators

Author: Dr. RĂ¼diger Paschotta

Cite the article using its DOI: https://doi.org/10.61835/tiz

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This articles discusses propagation modes of light in free space, in a transparent homogeneous medium, in a waveguide structure, or in an optical resonator. Alternatively, the term “mode” can also mean a mode of operation, e.g. continuous-wave mode locking, Q switching, or single-frequency operation; for such information, see the article on modes of laser operation.

When some light beam propagates in free space or in a transparent homogeneous medium, its transverse intensity profile generally changes during propagation (see Figure 1). There are, however, certain electric field distributions which are self-consistent during propagation; these are called *modes*. What “self-consistent” means in the mentioned definition, depends on the situation. Different situations are discussed in the following sections.

## Free-space Modes

### Plane Waves

The mathematically simplest kinds of modes in free space (or in an optically homogeneous medium) are *plane waves*. A plane wave satisfies the wave equation, provided only that the wavelength times the optical frequency matches the phase velocity of light in the medium. During propagation in a direction, a plane wave only changes its oscillation phase, and possibly its amplitude if there is optical loss or gain in a medium.

For a given optical frequency and a given optical medium, the wavenumber <$k$> of a plane wave is fixed, but different propagation directions are still possible. The continuum of plane waves with different propagation directions can be taken as a mathematical basis, which means that an arbitrary monochromatic field distribution can be regarded as a superposition of plane waves. Fourier transforms can be used for calculating such superpositions. As the plane waves are modes of free space, they are convenient for calculating the field propagation; this is a basis of Fourier optics.

### Gaussian, Hermite–Gaussian and Laguerre-Gaussian Modes

Although plane waves are mathematically very simple, they cannot resemble any wave occurring in reality, since they have an infinite transverse extent. Therefore, other kinds of modes, which are limited in the transverse spatial dimension, are often of higher interest. The simplest kind of such modes are *Gaussian modes*. A Gaussian beam expands or contracts during propagation, but is self-consistent in the sense that the amplitude profile is only scaled in the transverse dimension, but has a constant (in that case Gaussian) shape.

Each Gaussian mode is only the simplest member of a whole family of modes, which contains an infinite number of modes. The most frequently used mode families (mode systems) are those of *Hermite–Gaussian modes* and *Laguerre–Gaussian modes*. Within such a mode family, the Gaussian mode is the *fundamental mode*, while all other modes are called *higher-order modes* and have more complicated intensity profiles (see Figure 2). During propagation, the transverse extent of each higher-order mode changes in proportion to that of the fundamental mode.

The two mode indices indicate the number of zero crossings of the intensity distributions in horizontal and vertical direction, respectively.

Note that for each combination of an optical frequency, a beam axis, a focus position, and some beam radius of the Gaussian mode in the focus, a whole family e.g. of Hermite–Gaussian modes arises.

## Waveguide Modes

Waveguide structures are spatially inhomogeneous structures which can guide waves.
For light propagating in a waveguide, the self-consistency condition for a mode is more strict than for free-space modes: the shape of the complex amplitude profile in the transverse dimensions must remain exactly constant: any re-scaling is not allowed, only an overall phase change and a loss or gain of total optical power, which are both described by the *propagation constant*.

For a given optical frequency, a waveguide has only a finite number of *guided propagation modes*, the intensity distributions of which have a finite extent around the waveguide core. The number of guided modes, their transverse amplitude profiles and their propagation constants depend on the details of the waveguide structure and on the optical frequency. A single-mode waveguide (e.g. a single-mode fiber) has only a single guided mode per polarization direction. As an example of a multimode waveguide, Figure 3 shows the transverse profiles of all the LP modes of a multimode fiber.

The two colors indicate different signs of electric field values. The diagram has been generated with the **RP Fiber Power** software.

## Passive Fiber Optics

Part 2: Optical Fibers

We explain the basics of fiber modes, having self-reproducing amplitude profiles.

## Case Study: Mode Structure of a Multimode Fiber

We explore various properties of guided modes of multimode fibers. We also test how the mode structure of such a fiber reacts to certain changes of the index profile, e.g. to smoothening of the index step.

A waveguide also has *cladding modes*, the intensity distributions of which essentially fill the whole cladding (and core) region. Optical fibers (even single-mode fibers) have a large number of cladding modes, which often exhibit substantial propagation losses at the outer interface of the cladding.

Optical fibers (except for photonic crystal fibers) usually have a radially symmetric refractive index profile and also a relatively small refractive index contrast between core and cladding. In that case, one can quite accurately describes the mode as LP modes, which are mathematically simpler to describe and are therefore usually used in practice.

For radially symmetric refractive index profiles, there is also the interesting phenomenon of *orbital angular momentum modes* [5, 6]. Those carry an angular momentum which is *not* related to the photon spin, also not to a rotating polarization direction. The wavefronts exhibit a helical structure. This is possible only for modes having zero intensity at the beam center – for example, LP modes with non-zero <$l$>.

While for a plane wave propagating in a homogeneous medium the electric and magnetic fields are always both perpendicular to the propagation direction, this is not necessarily the case for waveguide modes. One distinguishes several situations:

- Transverse electromagnetic (TEM) modes have both electric and magnetic field perpendicular to the propagation direction. In other words, they have zero longitudinal field components in the direction of propagation, which is determined by the waveguide.
- Transverse electric (TE) modes have the electric field, but not the magnetic field perpendicular to the propagation direction. That means there is some longitudinal component of the magnetic field. They may also be called
*H modes*. - Transverse magnetic (TM) modes have the magnetic field, but not the electric field perpendicular to the propagation direction. That means there is some longitudinal component of the electric field. They may also be called
*E modes*. - Hybrid modes have non-zero electric and magnetic longitudinal field components.

Modes of fibers and other waveguides can be numerically calculated with so-called *mode solvers*, which can be part of a fiber simulation software. Depending on whether the waveguides have radially symmetric profiles and are weakly guiding, mode solver algorithms with a different level of complexity and quite different computation times are required. A mode solver for optical fibers, when restricted to pure LP modes, can be numerically much simpler and faster than a general 2D mode solver.

## Resonator Modes

For light in optical resonators (made of bulk-optical elements, not with waveguides), the self-consistency condition for a mode is again different: a mode must reproduce its exact transverse amplitude profile (without any re-scaling) only after a full resonator round trip; during the round trip, the mode profile may change in size and even in shape. On the other hand, the optical phase must also be reproduced after one round trip, i.e., the total experienced phase change must be an integer multiple of <$2\pi$>. The overall optical power may decrease or increase if there are optical losses or gain in the resonator.

Due to the phase condition, resonator modes can exist only for certain optical frequencies (the resonance frequencies). In general, the round-trip phase shift depends on the intensity pattern of a mode. Therefore, different higher-order modes can have different sets of mode frequencies. In the simpler case of a geometrically stable resonator, there are fundamental (axial) modes with Gaussian shape and higher-order transverse modes e.g. of Hermite–Gaussian shape. Unstable resonators also have modes, but with much more complicated mode properties.

The article on resonator modes gives more details.

## Application of the Mode Concept

In many photonic devices, light propagates only in a single mode. For example, single-mode operation of a laser means that only a single mode of its laser resonator is excited (i.e., carries a significant optical power). If it is truly a single mode, rather than a superposition of multiple axial modes, this also implies single-frequency operation. If the lasing mode is a Gaussian mode, the output is close to diffraction-limited, i.e. it has an ideal beam quality.

As another example, a single-mode fiber guarantees a fixed intensity profile at its output, assuming that all light launched into cladding modes (unguided modes) is lost before the fiber end is reached. The mode of a single-mode fiber normally has a shape which is similar to that of a Gaussian.

In other cases, it is often convenient to decompose all the propagating light into different modes. That decomposition means that for each mode some *mode amplitude* (a complex number, called a *phasor*) is calculated for the given light field, usually using some overlap integral. The basic advantage of such a procedure is that it is known how all the modes propagate: for each mode, there is only a phase change which can be calculated from its propagation constant, and possibly some change in optical power. The total intensity and phase profile can then be calculated for any position simply by adding up the contributions of different modes. This procedure can greatly simplify numerical simulations: a large number of amplitudes, resembling e.g. a two-dimensional optical field distribution with many samples on a fine grid, can be replaced with a relatively small number of mode amplitudes (excitation coefficients). That mode-based concept often strongly reduces the demands both in terms of required computer memory and computation time. Computation times are generally independent of the propagation distance.

The mode concept is useful even if the propagation conditions somewhat deviate from those for which the modes have been calculated. In such cases, mode coupling can occur: light from some mode can be coupled to one or several other modes. This is usually described with coupled differential equations for the mode amplitudes. Such mode coupling can be caused, e.g., by nonlinear interactions at high optical intensities or by external disturbances which act on a waveguide.

## More to Learn

- Case Study: Mode Structure of a Multimode Fiber
- Case Study: Telecom Fiber With Parabolic Index Profile

Encyclopedia articles:

Blog articles:

- The Photonics Spotlight 2006-12-03
- The Photonics Spotlight 2007-10-11
- The Photonics Spotlight 2008-04-15

### Bibliography

[1] | E. Snitzer, “Cylindrical dielectric waveguide modes”, J. Opt. Soc. Am. 51 (5), 491 (1961); https://doi.org/10.1364/JOSA.51.000491 |

[2] | D. Gloge, “Weakly Guiding Fibers”, Appl. Opt. 10 (10), 2252 (1971); https://doi.org/10.1364/AO.10.002252 |

[3] | A. Yariv, “Coupled-mode theory for guided-wave optics”, IEEE J. Quantum Electron. 9 (9), 919 (1973); https://doi.org/10.1109/JQE.1973.1077767 |

[4] | L. W. Casperson, “Mode stability of lasers and periodic optical systems”, IEEE J. Quantum Electron. 10 (9), 629 (1974); https://doi.org/10.1109/JQE.1974.1068485 |

[5] | L. Allen et al., “Orbital angular momentum of light and the transformation of Laguerre–Gaussian laser modes”, Phys. Rev. A 45 (11), 8185 (1992); https://doi.org/10.1103/PhysRevA.45.8185 |

[6] | M. J. Padgett, “Orbital angular momentum 25 years on”, Opt. Express 25 (10), 11265 (2017); https://doi.org/10.1364/OE.25.011265 |

[7] | P. T. Kristensen et al., “Modeling electromagnetic resonators using quasinormal modes”, Advances in Optics and Photonics 12 (3), 612 (2020); https://doi.org/10.1364/AOP.377940 |

[8] | R. Paschotta, tutorial on "Passive Fiber Optics", Part 2: Fiber Modes |

[9] | R. Paschotta, case study on fiber modes |

## Questions and Comments from Users

2020-09-09

What do TEM and LP stand for?

The author's answer:

TEM = transverse electromagnetic: electric and magnetic fields are perpendicular to the propagation direction.

LP = linearly polarized. That term is common for modes of optical fibers which are calculated under the assumption of a low refractive index contrast and a radially symmetric index profile.

2021-05-19

How to decompose a multi-mode fiber laser (or VCSELs) beam into modes, and get the amplitude weight of each?

The author's answer:

The first step is to determine an appropriate mode set. For example, it might be the guided modes of an optical fiber, and you apply the decomposition to the light which you focus onto the fiber input end.

The mode decomposition can numerically be done with overlap integrals, but for that you need the complex amplitude distribution of the input light – which is of course not easy to measure.

2022-11-08

Will RP Fiber Power solve the inverse problem: given a desired mode profile, calculate the index profile that will support it? If not, does any such software exist?

The author's answer:

This is not directly offered by RP Fiber Power, but using the script language one could implement an automatic optimization: vary the index profile such as to minimize the deviation from the wanted mode profile.

But it could also be done in a simpler and more direct way: take the radial equation for LP modes; with a known mode profile and its derivatives, you can directly calculate <$n(r)$>. That could of course also be implemented easily with our script language.

2023-03-26

As I understand it, when a single mode CW laser TEM_{00} mode is launched into a SMF fiber, it gets converted to LP_{01} mode. If that is the case, then how does this mode conversation work?

The author's answer:

Usually, the shape of the L_{01} mode is relatively similar to the Gaussian shape of such a laser beam. Therefore, you can efficiently couple the TEM_{00} mode output to the LP_{01} mode of the fiber. Some small part of the input optical power will get into the fiber cladding and will thus get lost. If you like, this is a kind of mode conversion by filtering.

2023-06-27

Is TEM mode the same as Hermite–Gaussian mode?

The author's answer:

No, not quite. A TEM mode is a mode having both electric and magnetic field perpendicular to the propagation direction. It could also be a waveguide mode which is not of Hermite–Gaussian form.

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2020-05-12

What is the relation between Laguerre–Gaussian and LP modes, having similar intensity patterns?

The author's answer:

LP modes are modes of optical fibers with a radially symmetric refractive index profile (and a week index contrast).

Laguerre–Gaussian modes are modes which are calculated for propagation in a homogeneous medium (for example free space).

Because the latter are based on calculations with polar coordinates, they look somewhat similar to LP modes.