Institute for Telecommunication Sciences
the research laboratory of the National Telecommunications and Information Administration

Hans J. Liebe; George A. Hufford; Michael G. Cotton

Abstract: Propagation characteristics of the atmosphere are modeled for the frequency range from 1 to 1000 GHz (1 THz) by the modular millimeter–wave propagation model MPM. Refractivity spectra of the main natural absorbers (i.e., oxygen, water–vapor, suspended droplets and ice particles) are computed from known meteorological variables. The primary contributions of dry air come from 44 O2 lines. Results from extensive 60–GHz laboratory measurements of the pressure–broadened O2 spectrum were applied to update the line data base. The water–vapor module considers 34 local H2O lines plus continuum contributions from the H2O spectrum above 1 THz, which are formulated as wing response of a pseudo–line centered at 1.8 THz. Cloud/fog effects are treated with the Rayleigh approximation employing revised formulations for the permittivities of water and ice. The influence of the Earth's magnetic field on O2 absorption lines becomes noticeable at altitudes between 30 and 120 km. Anisotropic medium properties result, which are computed by the Zeeman propagation model ZPM. Here the elements of a complex refractivity tensor are determined in the vicinity (+/-10 MHz) of O2 line centers and their effect on the propagation of plane, polarized radiowaves is evaluated. A spherically stratified (0 – 130 km) atmosphere provides the input for the codes MPM and ZPM in order to analyze transmission and emission properties of radio paths. Height profiles of air and water vapor densities and of the geocoded magnetic field are specified. ZPM predicts polarization– and direction–dependent propagation through the mesosphere. Emission spectra of the 9+ line (61150 +/- 3 MHz) for paths with tangential heights ranging from 30 to 125 km are consistent with data measured by the shuttle–based millimeter–wave limb sounder MAS.

Keywords: radio propagation; atmospheric propagation; millimeter-wave propagation model; mesospheric propagation


To request a reprint of this report, contact:

Lilli Segre, Publications Officer
Institute for Telecommunication Sciences
(303) 497-3572
LSegre@ntia.gov

For technical information concerning this report, contact:

Michael G. Cotton
Institute for Telecommunication Sciences
(303) 497-7346
mcotton@ntia.doc.gov


Disclaimer: Certain commercial equipment, components, and software may be identified in this report to specify adequately the technical aspects of the reported results. In no case does such identification imply recommendation or endorsement by the National Telecommunications and Information Administration, nor does it imply that the equipment or software identified is necessarily the best available for the particular application or uses.

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