Elliptical polarization

Elliptical polarization is the general form of polarization for transverse electromagnetic waves, in which the tip of the electric field vector traces an elliptical locus in the plane perpendicular to the propagation direction as the wave advances.^[1] This polarization state arises from the superposition of two orthogonal linear polarizations with the same frequency but differing in amplitude and phase.^[2] Specifically, elliptical polarization results from the superposition of two orthogonal linear polarizations with the same frequency and a phase difference neither 0° nor 180° (which would produce linear polarization); circular polarization is the special case with equal amplitudes and a ±90° phase difference.^[3] The handedness of elliptical polarization—whether left- or right-handed—is defined by the direction of rotation of the electric field vector when viewed against the direction of propagation, analogous to the conventions for circular polarization.^[1] It can also be conceptualized as the interference of left- and right-circularly polarized waves with unequal intensities, producing an elliptical trajectory rather than a circular one.^[2] In optical contexts, elliptical polarization is ubiquitous in natural light after interactions with anisotropic media, such as birefringent crystals or atmospheric scattering, and serves as the foundational description for analyzing wave behavior in three dimensions.^[4] Elliptical polarization plays a critical role in various applications, including the design of wave plates and polarizers that manipulate light for imaging, telecommunications, and spectroscopy.^[3] For instance, quarter-wave plates convert linear polarization to circular (or elliptical under adjusted conditions), enabling control over polarization states in laser systems and quantum optics experiments.^[2] Its study extends to astrophysics, where it reveals magnetic fields in celestial objects through the Zeeman effect,^[5] and to material science, where it probes chiral structures in thin films via phase retardation.^[6]

Fundamentals

Definition and Characteristics

Elliptical polarization is the general form of polarization for transverse electromagnetic waves, such as light, where the electric field vector traces an elliptical path in the plane perpendicular to the direction of propagation as the wave advances through one complete cycle. This occurs when the two orthogonal components of the electric field have different amplitudes and a phase difference other than zero or a multiple of 180 degrees (which would produce linear polarization). If the amplitudes are equal and the phase difference is exactly ±90 degrees, the result is circular polarization, a special case of elliptical polarization. The resulting ellipse defines the polarization state, distinguishing it from other forms by its curved trajectory.^[7]^[8] Key characteristics of elliptical polarization include the orientation of the ellipse's major and minor axes, which determine the tilt relative to the propagation direction, and the axial ratio, expressing the ratio of the major to minor axis lengths. The polarization also possesses handedness, classified as left-handed or right-handed based on the rotation direction of the electric field vector when viewed along the propagation direction: right-handed if the rotation follows the right-hand rule (thumb in propagation direction, fingers curling in rotation sense), and left-handed otherwise. Elliptical polarization includes linear polarization as a limiting case, where the phase difference causes the ellipse to degenerate into a straight line along one axis, and circular polarization as another limit, where the axes are equal in length, resulting in a circle.^[9]^[10] Physically, the tip of the electric field vector varies in amplitude while rotating along the elliptical path over time, leading to distinct observable effects such as non-uniform intensity variations when the elliptically polarized wave interacts with linear polarizers or analyzers at different orientations. This behavior arises because the projection of the rotating vector onto the polarizer's transmission axis changes periodically, producing maxima and minima that depend on the ellipse's parameters. Such implications are crucial in applications involving polarization-sensitive detection, where the non-uniform patterns reveal the underlying elliptical state.^[11]^[3] The concept of elliptical polarization was first rigorously described by Augustin-Jean Fresnel in his 1822 memoir on double refraction in quartz crystals, as part of developing the wave theory of light, where he introduced the terminology alongside linear and circular forms to explain observed birefringence phenomena.^[12]

Relation to Linear and Circular Polarization

Elliptical polarization is the most general form of polarization for electromagnetic waves, where the electric field vector traces an elliptical path, and both linear and circular polarizations emerge as limiting cases of this configuration.^[10] Linear polarization represents a special case of elliptical polarization in which the ellipse collapses into a straight line, causing the electric field to oscillate along a fixed direction without rotation. This degeneration occurs when the phase difference between the two orthogonal components of the electric field is 0 or π radians.^[13]^[14] Circular polarization is another special case, where the ellipse becomes a circle due to equal lengths of the major and minor axes, resulting in the electric field rotating at a constant magnitude. This state is realized with a phase difference of ±π/2 radians between the orthogonal components and equal amplitudes.^[15]^[13] The elliptical form generally results from the superposition of two orthogonal linear polarization components having an arbitrary ratio of amplitudes and a phase difference between 0 and π/2 radians. As these parameters vary—such as increasing the phase difference from 0 toward π/2 while adjusting amplitudes—the polarization ellipse transitions smoothly from a linear configuration (degenerate ellipse as a line) through intermediate elliptical shapes to a circular one, as illustrated in diagrams depicting the evolving trajectory of the electric field vector's tip.^[14]^[10] These polarizations differ physically in the motion of the electric field vector: linear polarization involves no rotation, with the vector reversing direction along a single axis; circular polarization features uniform rotation at constant speed and field strength; and elliptical polarization exhibits a rotational path with varying field magnitude and speed, as the vector traces the ellipse's perimeter between its major and minor axes.^[15]^[10]

Mathematical Representation

Jones Calculus Description

The Jones calculus provides a vector-based mathematical framework for describing the polarization state of coherent, monochromatic light using complex amplitudes of the electric field components. Developed by R. Clark Jones in 1941, this formalism represents the electric field as a two-component complex vector \mathbf{E} = \begin{pmatrix} E_x \\ E_y \end{pmatrix}, where E_x = a e^{i \delta_x} and E_y = b e^{i \delta_y} denote the x- and y-polarized components, with a and b as real amplitudes and \delta_x, \delta_y as their respective phases.^[16]^[17] This representation captures both the relative amplitudes and phase differences essential for elliptical polarization. For a general elliptical polarization state, the Jones vector is determined by arbitrary positive amplitudes a and b, along with the phase difference \Delta = \delta_y - \delta_x. When a \neq b and $0 < |\Delta| < \pi/2 (or \pi/2 < |\Delta| < \pi), the resulting trajectory of the electric field vector traces an ellipse in the xy-plane. The handedness of this elliptical polarization—whether right-handed (clockwise rotation when looking toward the source) or left-handed (counterclockwise)—is governed by the sign of \Delta: a negative \Delta (e.g., -\pi/2) yields right-handed ellipticity, while a positive \Delta (e.g., +\pi/2) produces left-handed ellipticity.^[17]^[18] Jones vectors for pure polarization states are typically normalized to unit length, ensuring |E_x|^2 + |E_y|^2 = 1, which corresponds to a total intensity of unity. For instance, the normalized Jones vector for right-circular polarization (a special case of elliptical polarization with a = b and \Delta = -\pi/2) is \frac{1}{\sqrt{2}} \begin{pmatrix} 1 \\ -i \end{pmatrix}, while left-circular is \frac{1}{\sqrt{2}} \begin{pmatrix} 1 \\ i \end{pmatrix}.^[17]^[18] Transformations of elliptical states under optical elements, such as retarders, are handled via matrix multiplication in Jones calculus. A quarter-wave plate, which introduces a \pi/2 phase shift between orthogonal components, converts linearly polarized light into elliptical polarization. For example, applying a quarter-wave plate with its fast axis along x to linearly polarized light at 45° (Jones vector \frac{1}{\sqrt{2}} \begin{pmatrix} 1 \\ 1 \end{pmatrix}) yields the right-circular state \frac{1}{\sqrt{2}} \begin{pmatrix} 1 \\ -i \end{pmatrix}, using the plate's Jones matrix \begin{pmatrix} e^{i\pi/4} & 0 \\ 0 & e^{-i\pi/4} \end{pmatrix} (up to a global phase).^[16]^[17]^[18]

Stokes Parameters and Poincaré Sphere

The Stokes parameters provide a set of four real-valued quantities that fully characterize the polarization state of light, including elliptical polarization, based on measurable intensities rather than complex field amplitudes.^[19] These parameters, originally introduced by George Gabriel Stokes in 1852 and adapted for optical polarization, are defined for a monochromatic electromagnetic wave with electric field components E_x and E_y as follows:

\begin{align} S_0 &= |E_x|^2 + |E_y|^2, \\ S_1 &= |E_x|^2 - |E_y|^2, \\ S_2 &= 2 \operatorname{Re}(E_x E_y^*), \\ S_3 &= 2 \operatorname{Im}(E_x E_y^*), \end{align}

where S_0 represents the total intensity, S_1 the difference between horizontal and vertical linear polarizations, S_2 the difference between linear polarizations at \pm 45^\circ, and S_3 the difference between right- and left-circular polarizations.^[19] For fully polarized light, the parameters satisfy S_0^2 = S_1^2 + S_2^2 + S_3^2, while the degree of polarization is given by P = \sqrt{S_1^2 + S_2^2 + S_3^2}/S_0 \leq 1.^[19] The Stokes parameters relate directly to the geometric properties of the polarization ellipse. The orientation angle \psi (tilt of the major axis) and ellipticity angle \chi (related to the axial ratio by \tan \chi = b/a, where a and b are the semi-major and semi-minor axes) are derived from combinations of the parameters: \tan(2\psi) = S_2 / S_1 and \sin(2\chi) = S_3 / S_0.^[20] These relations allow the ellipse's shape and orientation to be determined solely from intensity measurements, providing a practical bridge between observable quantities and the underlying polarization state.^[20] The Poincaré sphere offers a geometric visualization of the Stokes parameters on a three-dimensional unit sphere, where fully polarized states correspond to points on the surface with S_0 = 1 and the vector (S_1, S_2, S_3) as Cartesian coordinates.^[21] Introduced by Henri Poincaré in 1892 to track polarization transformations through optical media, the sphere maps the azimuthal angle $2\psi and polar angle $2\chi such that the equator (\chi = 0) represents all linear polarizations, the north pole (\chi = +45^\circ) right-circular polarization, the south pole (\chi = -45^\circ) left-circular polarization, and intermediate latitudes elliptical polarizations.^[22]^[21] Operations like retarders or rotators appear as rotations on the sphere, simplifying analysis of polarization evolution.^[22] A key advantage of the Stokes parameters is their ability to describe partially polarized light, where P < 1, by representing the state as a point inside the Poincaré sphere, unlike Jones vectors which apply only to fully coherent, purely polarized fields.^[23] This extends naturally to the Mueller calculus, where polarization transformations are handled via 4×4 real matrices acting on the Stokes vector, enabling robust modeling of depolarizing systems in optics and remote sensing.^[23]

Polarization Ellipse Geometry

Ellipse Parameters

The polarization ellipse describes the trajectory traced by the tip of the electric field vector of an elliptically polarized electromagnetic wave in the plane transverse to its propagation direction. The ellipse is characterized by its major and minor axes, with lengths denoted as 2a and 2b respectively, where a > b ≥ 0 represents the semi-major and semi-minor axes.^[14] These axes determine the extent of the field oscillation along the principal directions of the ellipse.^[24] The area enclosed by the polarization ellipse is given by πab, which provides a geometric measure related to the wave's intensity; specifically, the total intensity is proportional to a² + b², while the product ab reflects the degree of ellipticity.^[14] The orientation of the ellipse is specified by the angle ψ, which measures the tilt of the major axis relative to a reference x-axis in the transverse plane, with ψ ranging from 0 to π.^[24] This angle fully captures the rotational position of the ellipse without ambiguity due to the π-periodicity of polarization states.^[14] The shape of the ellipse is quantified by the ellipticity angle χ, defined such that

\tan \chi = \frac{b}{a},

where χ ranges from -π/4 to π/4.^[24] The value χ = 0 corresponds to linear polarization, where b = 0 and the ellipse degenerates to a line segment along the major axis, while χ = ±π/4 indicates circular polarization, with a = b and the ellipse becoming a circle.^[24] The sign of χ distinguishes the handedness of the rotation.^[14] Certain properties of the polarization ellipse remain invariant regardless of the observer's frame. The time-averaged Poynting vector, which represents the direction and magnitude of energy flow, lies along the propagation direction and is thus perpendicular to the plane of the ellipse.^[25] Additionally, the geometric parameters a, b, ψ, and χ are defined solely within the transverse plane and exhibit no dependence on the propagation direction itself.^[26]

Orientation and Axial Ratio

The axial ratio (AR) quantifies the degree of ellipticity in the polarization ellipse by measuring the asymmetry between its major axis length a and minor axis length b, defined as AR = a/b where AR \geq 1. This ratio serves as a direct indicator of eccentricity: an AR of 1 corresponds to perfect circular polarization, while values approaching infinity describe linear polarization. In practical terms, AR influences propagation through birefringent media, where the relative phase shifts between orthogonal components modify the output AR, leading to observable changes in polarization state that depend on the material's refractive index differences.^[27]^[28] In antenna engineering, AR is essential for minimizing polarization mismatch losses, which occur when the transmitted or received wave's ellipticity deviates from the antenna's design specification, reducing signal efficiency. For circularly polarized antennas, maintaining AR below 3 dB ensures mismatch losses under 0.25 dB, enabling robust performance in systems like satellite communications where environmental factors can degrade polarization purity.^[29] The orientation angle \psi describes the directional tilt of the polarization ellipse, representing the angle between the major axis and a reference axis (typically the x-axis). It is calculated from the Jones vector components E_x and E_y as

\psi = \frac{1}{2} \arctan\left( \frac{2 \Re(E_x E_y^*)}{|E_x|^2 - |E_y|^2} \right),

where \Re denotes the real part; this formulation arises from the geometry of the electric field projections and determines how the ellipse aligns with the propagation coordinate system. The value of \psi affects diffraction patterns in optical setups, as misalignment between the ellipse orientation and structural features like gratings or apertures alters the scattered intensity and angular distribution.^[30]^[31] Elliptical polarization's handedness is intrinsically tied to the sign of the ellipticity angle \chi, with positive \chi indicating right-handed rotation (clockwise) and negative \chi left-handed (counterclockwise), where \tan \chi = b/a. This linkage governs interactions in chiral media, such as optical rotatory dispersion or circular dichroism, where opposite handedness produces distinct interference effects, including asymmetric transmission or enhanced absorption due to the medium's structural chirality. The basic ellipse axes a and b provide the foundation for these parameters, as referenced in prior geometric discussions.^[24]^[18]

Generation and Manipulation

Production Methods

Elliptical polarization can be generated from linearly polarized light using birefringent wave plates, which introduce a phase delay between orthogonal polarization components. A quarter-wave plate oriented at 45° to the input linear polarization axis produces circular polarization, a special case of elliptical polarization where the major and minor axes of the ellipse are equal.^[32] For general elliptical states, an arbitrary retarder with a phase delay other than π/2 radians is used; the ellipticity and orientation depend on the retarder's fast axis angle relative to the input polarization.^[33] A common setup involves a linear polarizer followed by a birefringent plate, such as a wave plate, to create elliptical polarization from unpolarized light. The polarizer first produces linear polarization, after which the plate introduces a phase delay Δ between the ordinary and extraordinary rays, with the plate's optic axis at an angle θ to the polarizer's transmission axis; varying Δ and θ controls the ellipse's axial ratio and tilt.^[10] Liquid crystal devices enable tunable elliptical polarization through voltage-controlled birefringence. In a liquid crystal variable retarder (LCVR), an applied electric field alters the molecular alignment, changing the effective birefringence and thus the phase retardation; this allows real-time adjustment of ellipticity from linearly polarized input beams.^[34] In quantum optics, entangled photon pairs exhibiting elliptical polarization states can be produced via spontaneous parametric down-conversion (SPDC) in nonlinear crystals. A pump laser induces the process in a birefringent crystal like beta-barium borate, generating photon pairs whose joint polarization is inherently elliptical, tunable by the pump's polarization and crystal orientation; such states are useful for quantum information protocols.^[35]

Detection and Analysis Techniques

Detection and analysis of elliptical polarization involve specialized instruments that quantify the orientation, axial ratio, and handedness of the polarization ellipse, often by measuring the associated Stokes parameters. Polarimeters are fundamental tools for this purpose, enabling the characterization of arbitrary polarization states, including elliptical ones, through intensity measurements at various orientations.^[36] A classic polarimeter configuration employs a rotating quarter-wave plate followed by a linear analyzer and photodetector. As the quarter-wave plate rotates, it modulates the input elliptical polarization into varying linear components, producing a intensity signal at the detector whose amplitude and phase reveal the Stokes parameters, from which the ellipse parameters—such as major axis orientation and ellipticity angle—can be derived. This method achieves high accuracy for monochromatic light, with modulation frequencies at 2ω and 4ω for a plate rotating at angular speed ω, allowing separation of DC and AC components to isolate polarization information.^[36]^[37] Self-calibrating variants of this setup minimize errors from misalignment by incorporating motorized rotation of both the waveplate and analyzer, ensuring robust measurement of elliptical states across visible wavelengths. For spatially resolved analysis, imaging polarimetry utilizes charge-coupled device (CCD) arrays integrated with micropolarizer filters. These systems divide the focal plane into sub-pixels covered by linear polarizers and quarter-wave retarders oriented at 0°, 45°, 90°, and 135°, enabling simultaneous capture of the four Stokes parameters for each image point. This facilitates mapping of elliptical polarization distributions, such as in birefringent samples, where the axial ratio and orientation vary spatially, with resolutions down to micrometers depending on the array pitch.^[38] Near-infrared implementations extend this to full-Stokes imaging, supporting ellipse characterization in low-light conditions typical of scientific microscopy.^[38] Ellipsometry provides a reflectance-based approach particularly suited for thin-film characterization, where incident linearly polarized light reflects into an elliptical state due to the film's optical properties. The technique measures the amplitude ratio ψ (tan ψ = |r_p / r_s|, where r_p and r_s are the complex reflection coefficients for p- and s-polarizations) and phase difference Δ between these components, directly yielding the polarization ellipse parameters for the reflected beam. Null ellipsometers, using rotating polarizers to achieve minimum intensity, offer precision for film thicknesses from nanometers to microns, while spectroscopic variants scan wavelengths to map dispersion effects on the ellipse.^[39]^[40] This method excels in non-destructive analysis of dielectric layers, with ψ and Δ sensitivities to 0.01° and 0.1°, respectively, enabling inference of refractive index and thickness.^[39] Modern division-of-amplitude polarimeters (DOAPs) enable real-time measurement of elliptical parameters using Wollaston prisms to split the input beam into orthogonally polarized components. In a typical setup, a beam splitter divides the light into two beams, each of which is incident on a Wollaston prism that separates the s- and p-components onto separate linear photodetectors, providing instantaneous Stokes vectors and thus axial ratio (AR = major/minor axis) and orientation angle θ. These instruments operate broadband from visible to near-infrared, with response times under 1 ms, making them ideal for dynamic polarization monitoring without mechanical rotation.^[41]^[42] Uncoated birefringent crystals in the prisms minimize chromatic dispersion, ensuring accurate AR and θ retrieval for elliptical inputs with ellipticities up to 45°.^[41]

Applications

In Optical Systems

In liquid crystal displays (LCDs), elliptical polarization plays a crucial role in the operation of twisted nematic (TN) structures, where the liquid crystal molecules are arranged in a helical configuration that rotates the polarization state of incoming linearly polarized light into elliptical states as it propagates through the device. This ellipticity arises from the birefringence induced by the twisted alignment, allowing the light to be modulated effectively when passing through crossed polarizers, thereby enabling the grayscale and color control essential for display functionality. The eigenvectors of the TN-LCD are inherently elliptically polarized, with the degree of ellipticity varying with the applied voltage and the device's birefringence, which optimizes light transmission and contrast ratios.^[43]^[44] For laser beam shaping in fiber optic systems, maintaining elliptical polarization is vital to minimize mode coupling losses, particularly in high-power applications where polarization fluctuations can lead to energy transfer between orthogonal modes, degrading beam quality and efficiency. Elliptical cladding or core polarization-maintaining fibers are engineered with asymmetric stress rods or geometric ellipticity to preserve the input elliptical state over long propagation distances, ensuring stable beam profiles for precise shaping and focusing in optical delivery systems. This preservation reduces insertion losses by up to several decibels compared to standard single-mode fibers and supports applications in laser processing and medical optics by preventing depolarization-induced scattering.^[45]^[46] In holography, encoding elliptical polarization enables the creation of three-dimensional vectorial images that incorporate both amplitude and polarization information, allowing for advanced security features based on the handedness of the ellipse. By recording the full Stokes parameters of elliptical states, holograms can reconstruct 3D scenes with spatially varying polarization, where the left- or right-handed ellipticity acts as an optical key, rendering the image invisible or distorted under incorrect polarization illumination. This vectorial approach enhances data capacity and anti-counterfeiting measures, as demonstrated in metasurface-based holograms that support arbitrary elliptical states for secure, high-fidelity 3D visualization.^[47]^[48] Metamaterials facilitate polarization conversion, including from linear to cross-polarized states, through artificial nanostructures that manipulate the phase and amplitude of orthogonal field components, enabling tailored electromagnetic responses for stealth technologies. These structures, often composed of split-ring resonators or anisotropic meta-atoms, achieve controlled birefringence to redirect scattered energy in microwave frequencies. In stealth applications, such as radomes, this conversion suppresses radar reflections while maintaining transparency for operational signals.^[49]^[50]

In Communication and Sensing

In satellite communications, elliptical polarization is employed in antenna design to mitigate signal fading caused by ionospheric Faraday rotation, which rotates the polarization plane of linearly polarized waves and leads to deep fades when the received polarization mismatches the receiver. By transmitting signals with elliptical or near-circular polarization, the system maintains more consistent signal integrity regardless of rotation angle, as the rotating ionosphere affects the ellipse parameters but does not convert it to orthogonal states that cause severe loss. This approach is particularly beneficial for geostationary satellite links operating below 10 GHz, where ionospheric effects are pronounced.^[51] In radar systems, dual-polarization techniques enhance weather discrimination by measuring differential reflectivity and depolarization ratios, allowing differentiation between rain and hail based on hydrometeor shape and orientation. For instance, oblate raindrops produce positive differential reflectivity, while more spherical or irregular hail results in near-zero or negative values. This technique, implemented in polarimetric weather radars, also aids in identifying non-meteorological echoes, such as birds or insects, through depolarization signatures. Fiber-optic communications leverage polarization-division multiplexing (PDM) with controlled elliptical polarization states to transmit two orthogonal channels on the same wavelength, effectively doubling bandwidth without additional spectrum. Elliptical core fibers maintain polarization stability over long distances, minimizing crosstalk in high-speed systems exceeding 100 Gb/s, where dynamic polarization controllers adjust ellipticity to compensate for birefringence-induced rotation. This method enhances spectral efficiency in dense wavelength-division multiplexing networks.^[52]^[53] In biomedical sensing, Mueller matrix imaging exploits changes in light ellipticity induced by tissue scattering to detect cancerous alterations, as malignant cells exhibit distinct depolarization and retardance compared to healthy tissue. By analyzing the full Mueller matrix, which quantifies transformations including elliptical components, this technique identifies ellipticity shifts in collagen-rich stroma. Seminal studies on human tissue samples highlight its potential for early-stage detection, with quantitative parameters like the degree of polarization correlating to tumor grade.

Natural Occurrences

Astrophysical Examples

One prominent example of elliptical polarization in astrophysics arises from synchrotron radiation emitted by relativistic electrons spiraling in magnetic fields, as observed in supernova remnants like the Crab Nebula. In this pulsar wind nebula, the radiation exhibits a high degree of linear polarization approaching 20-30% in X-rays, corresponding to highly elliptical states with axial ratios greater than 10 due to the small circular component from the finite pitch angles of electron trajectories.^[54] This polarization signature, first identified in radio observations and later confirmed in X-ray data, provides insights into the ordered magnetic field structure within the nebula.^[55] Stellar magnetic fields manifest elliptical polarization through the Zeeman effect, where spectral line splitting in the presence of longitudinal fields produces circularly polarized components, a special case of elliptical polarization measurable via the Stokes V parameter. In chemically peculiar stars and white dwarfs, transverse fields contribute linear components that combine with circular ones to yield net elliptical polarization, enabling mapping of field strengths up to several kilogauss.^[56] Observations of such effects in Ap stars reveal complex field topologies, with elliptical polarization degrees reflecting the interplay between Zeeman splitting and atomic absorption.^[57] Recent Atacama Large Millimeter/submillimeter Array (ALMA) observations from the 2020s have detected elliptical polarization patterns in protoplanetary disks, attributed to the alignment of dust grains with respect to magnetic fields or radiative torques. In inclined disks like HL Tau, the polarization exhibits an elliptical morphology at millimeter wavelengths, resulting from aerodynamic alignment where grains rotate differently from the gas, producing fractional polarization up to 1-2%.^[58] Such signatures in systems like AS 209 confirm grain growth and settling, linking polarization to disk dynamics essential for planet formation.^[59]

Atmospheric and Environmental Phenomena

In the Earth's atmosphere, elliptical polarization of light primarily arises from deviations in scattering processes beyond ideal single Rayleigh scattering, which produces purely linear polarization. Multiple scattering events among air molecules and aerosols introduce phase differences between orthogonal electric field components, resulting in elliptical components in skylight. Early measurements confirmed the presence of small but detectable elliptical polarization in the day sky, with the degree of ellipticity varying by solar zenith angle and atmospheric clarity, challenging the classical Rayleigh model. In aerosol-rich conditions, such as hazy skies, scattering by polydisperse spherical particles further enhances ellipticity due to mean phase shifts in the scattered wavefront, leading to partial circular components within the elliptical state. Environmental phenomena involving interfaces between media also generate elliptical polarization naturally. Total internal reflection at air-water boundaries, as occurs with submerged air bubbles, produces significant elliptical polarization in the reflected light, with the handedness and axial ratio depending on the angle of incidence relative to the critical angle (approximately 48.6° for water-air). This effect is observable in stationary bubbles and propagating waves on bubble surfaces, providing a rare high-degree source of elliptical light in aquatic settings.^[60] Similarly, oblique scattering from rough surfaces can yield elliptical polarization through asymmetric reflection of incident linearly polarized skylight.^[61] In underwater environments, the polarization of downwelling skylight becomes elliptically modified near the surface due to refraction at the water-air interface and the interaction with the linearly polarized atmospheric light field. This submarine elliptical polarization is most pronounced within a few centimeters of the surface and along sightlines near the critical angle, with the degree decreasing rapidly with depth and wavelength.^[62] These atmospheric and environmental effects highlight how elliptical polarization emerges from complex interactions in natural scattering and reflection, influencing visibility and potential navigational cues for organisms.