Substrate-Integrated Millimeter-Wave Antennas for Next-Generation Communication and Radar Systems. Группа авторов

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with diffraction or reflection, in particular at lower frequencies such as VHF and below.

      On the other hand, like a light wave, also an electromagnetic wave, the mmWs with shorter wavelengths in millimeter orders, in particular, at EHF and above, always propagate in LOS modes. Their propagation is significantly affected by the typical phenomena of reflection, refraction, diffraction, absorption, and scattering so that a clear path without any lossy or/and wavelength comparable obstacles in the traveling path is required. Such a propagation feature of waves will be reflected in the design considerations of antennas in mmW systems.

Frequency Wavelength in air Dominate propagation modes Typical applications
Extremely low frequency (ELF): 3–30 Hz 9993.1–99 930.8 km Guided between the Earth and the ionosphere Very long‐distance wireless communication (under water/ground)
Super low frequency (SLF): 30–300 Hz 999.3–9993.1 km Guided between the Earth and the ionosphere Very long‐distance wireless communication (under water/ground)
Ultra low frequency (ULF): 300–3000 Hz 99.9–999.3 km Guided between the Earth and the ionosphere Very long‐distance wireless communication (under water/ground)
Very low frequency (VLF): 3–30 kHz 10.0–99.9 km Guided between the Earth and the ionosphere Very long‐distance wireless communication (under water/ground)
Low frequency (LF): 30–300 kHz 1.0–10.0 km Guided between the Earth and the ionosphere; ground guided Very long‐distance wireless communication and broadcasts
Medium frequency (MF): 300–3000 kHz 0.1–1.0 km Ground guided; refracted wave in ionospheric layers Very long‐distance wireless communication and broadcasts
High frequency (HF): 3–30 MHz 10.0–100.0 m Ground guided; refracted wave in ionospheric layers Very long‐distance wireless communication and broadcasts
Very high frequency (VHF): 30–300 MHz 1.0–10.0 m Line‐of‐sight refracted in ionospheric Wireless communication, radio, and television broadcasts
Ultra high frequency (UHF): 300–3000 MHz 0.1–1.0 m Line‐of‐sight Wireless communication, television broadcasts, heating, positioning, remote controlling
Super high frequency (SHF): 3–30 GHz 10.0–100.0 mm Line‐of‐sight Wireless communication, direct satellite broadcasts, radio astronomy, radar
Extremely high frequency (EHF): 30–300 GHz 1.0–10.0 mm Line‐of‐sight Wireless communication, radio astronomy, radar, remote sensing, energy weapon, scanner
Tremendously high frequency (THF): 300–3000 GHz 0.1–1.0 mm Line‐of‐sight Radio astronomy, remote sensing, imaging, spectroscopy, wireless communications

      The wave attenuation is caused by the absorption of water (H2O) and/or oxygen (O2) in the atmosphere. There are several absorption peaks across the frequency band up to 400 GHz. The lowest two peaks appear around the 25 and 60 GHz bands, respectively. In particular, the attenuation at the 60 GHz band is 10 times that of the 30 GHz band. In addition, the temperature, pressure, and water vapor density also significantly affect the absorption. It suggests that the wave attenuation at the mmW bands may increase greatly when it is raining, snowing, or foggy. Such an observation must be considered in the calculation of link budget of mmW systems. As a result, the selection and design of antennas should meet the requirements of mmW systems with particular attention to uniqueness of wave propagation.

      1.3.1 Important Features

      With the shorter operating wavelengths, mmW systems also

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