Backscatter
In physics, backscatter is the reflection of waves, particles, or signals back to the direction from which they came. It is usually a diffuse reflection due to scattering, as opposed to specular reflection as from a mirror, although specular backscattering can occur at normal incidence with a surface. Backscattering has important applications in astronomy, photography, and medical ultrasonography. The opposite effect is forward scatter, e.g. when a translucent material like a cloud diffuses sunlight, giving soft light.
Backscatter of waves in physical space
Backscattering can occur in quite different physical situations, where the incoming waves or particles are deflected from their original direction by different mechanisms:- Diffuse reflection from large particles and Mie scattering, causing alpenglow and gegenschein, and showing up in weather radar;
- Inelastic collisions between electromagnetic waves and the transmitting medium, important in fiber optics, see below;
- Elastic collisions between accelerated ions and a sample
- Bragg diffraction from crystals, used in inelastic scattering experiments ;
- Compton scattering, used in Backscatter X-ray imaging.
- Stimulated backscatter, observed in non-linear optics, and described by a class of solutions to the three-wave equation.
- in X-ray imaging, backscattering means just the opposite of transmission imaging;
- in inelastic neutron or X-ray spectroscopy, backscattering geometry is chosen because it optimizes the energy resolution;
- in astronomy, backscattered light is that which is reflected with a phase angle of less than 90°.
- In alpenglow, red light prevails because the blue part of the spectrum is depleted by Rayleigh scattering.
- In gegenschein, constructive interference might play a role.
- Coherent backscattering is observed in random media; for visible light most typically in suspensions like milk. Due to weak localization, enhanced multiple scattering is observed in back direction.
- * The Back Scattering Alignment coordinate system is often used in radar applications
- * The Forward Scattering Alignment coordinate system is primarily used in optical applications
Radar, especially weather radar
Backscattering is the principle behind radar systems. In weather radar, backscattering is proportional to the 6th power of the diameter of the target multiplied by its inherent reflective properties, provided the wavelength is larger than the particle diameter. Water is almost 4 times more reflective than ice but droplets are much smaller than snow flakes or hail stones. So the backscattering is dependent on a mix of these two factors. The strongest backscatter comes from hail and large graupel due to their sizes, but non-Rayleigh effects can confuse interpretation. Another strong return is from melting snow or wet sleet, as they combine size and water reflectivity. They often show up as much higher rates of precipitation than actually occurring in what is called a brightband. Rain is a moderate backscatter, being stronger with large drops and much weaker with small droplets. Snow has rather weak backscatter. Dual polarization weather radars measure backscatter at horizontal and vertical polarizations to infer shape information from the ratio of the vertical and horizontal signals.In waveguides
The backscattering method is also employed in fiber optics applications to detect optical faults. Light propagating through a fiber-optic cable gradually attenuates due to Rayleigh scattering. Faults are thus detected by monitoring the variation of part of the Rayleigh backscattered light. Since the backscattered light attenuates exponentially as it travels along the optical fiber cable, the attenuation characteristic is represented in a logarithmic scale graph. If the slope of the graph is steep, then power loss is high. If the slope is gentle, then optical fiber has a satisfactory loss characteristic.The loss measurement by the backscattering method allows measurement of a fiber-optic cable at one end without cutting the optical fiber hence it can be conveniently used for the construction and maintenance of optical fibers.