Policy on Intellectual Property Right (IPR)
1 Introduction
2 Atmospheric conditions in the 67-116 GHz (3-4 mm) range
2.1 Free-space transmission loss
2.2 Atmospheric attenuation characteristics in the 67-116 GHz (3-4
mm) range
2.3 Terrain shielding, clutter and other sources of attenuation
3 Sharing and protection requirements in 67-116 GHz range
4 Scientific motivation
4.1 Unveiling the formation of Solar System analogues on
terrestrial scale
4.2 Probing the initial conditions for planetary systems and life
with astrochemistry
4.3 Charting the assembly, structure and evolution of galaxies from
the first billion years to the present
4.4 Understanding the formation and evolution of stellar and
supermassive black holes in the era of multi-messenger astronomy
5 Radio telescopes operating in the 67-116 GHz (3-4 mm) range
5.1 Summary of facilities
5.2 Receiver technology
5.3 Antenna beam pattern
6 References and Related ITU-R documents
7 List of acronyms and abbreviations