Coherent non-linear optics — recent advances: Edited by M.S. Feld, V.S. Letokhov Springer-Verlag, 1980, pp 377 + xviii, $49

Abstract

Millimeter and submillimeter-wave observations provide important information for the studies of atmospheric chemistry and astrochemistry (molecular clouds, stars formation, galactic study, comets and cosmology). But, these observations depend strongly on instrumentation techniques and on the site quality. New techniques or higher detector performances result in unprecedented observations and, sometimes, the observational needs drive developments of new detector technologies, for example, superconducting junctions (SIS mixers) because of their high sensitivity in heterodyne detection in the millimeter and submillimeter wave range (100–700 GHz), HEB (Hot Electron Bolometer) mixers which are being developed by several groups for application in THz observations. For the sub-millimetre wavelengths heterodyne receivers, the local oscillator (LO) is still a critical element. So far, solid state fundamental sources are often not powerful enough for most of the applications at millimetre or submillimetre wavelengths: large efforts using new planar components (HBV) and integrated circuits, or new technics (laser mixing) are now in progress, in a few groups.The new large projects as SOFIA, FIRST, ALMA, … for astronomy; SMILES, EOS-MLS, … for aeronomy and other projects for the planetary science (ROSETTA, Mars Explorer, …), will benefit of the new developments.Les observations en ondes millimétriques et submillimétriques fournissent des informations importantes pour l'étude de la chimie atmosphérique et de l'astrochimie (nuages moléculaires, formation des étoiles, étude des galaxies, des comètes) et la cosmologie. Mais ces observations dépendent très fortement des techniques instrumentales mises en œuvre et de la qualité des sites.