108112MHz

108112MHz refers to a frequency of 108.112 gigahertz (GHz) in the electromagnetic spectrum. At this value, the signal lies in the extremely high frequency (EHF) band, which spans roughly from 30 GHz to 300 GHz. Frequencies in this region are used primarily for specialized applications rather than general consumer broadcasting.

In practice, 108.112 GHz and nearby frequencies are utilized in fields such as radio astronomy, where millimeter-wavelength observations probe molecular gas and dust in space. The band is also relevant to scientific research and certain high-capacity communication experiments, including satellite links and point-to-point backhaul under licensed allocations in some regions. Weather radar and atmospheric studies may exploit portions of nearby millimeter-wave spectra as well.

Propagation at about 108 GHz is characterized by strong atmospheric absorption, particularly from water vapor and oxygen, and by sensitivity to weather conditions. Signals at these frequencies require clear line of sight, precise pointing, and high-performance, often cryogenically cooled receivers. Antenna systems typically rely on high-gain dishes and sophisticated transmitter–receiver hardware to overcome significant path losses.

Regulatory allocation for 108.112 GHz is governed by international and national authorities, such as the International Telecommunication Union and regional regulators. Because the band is tightly managed and experiences strong environmental attenuation, deployments are usually niche, planned, and licensed, rather than common commercial services.

Overall, 108112MHz occupies a specialized segment of the spectrum used mainly for scientific, research, and select high-frequency communication activities rather than everyday broadcasting.