Millimeter astronomy - Open Access .click

S-MTT International Microwave Symposium Digest, 1974
Millimeter wave receivers are discussed from the point of view of applications of line astronomy. A heterodyne bolometer system is described which has a noise temperature of 300/spl deg/K at 230 GHz. It is expected that these receivers will extend the range of radio line astronomy to about 500 GHz.
T.G. Phillips, K.B. Jefferts
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Molecular Millimeter Wave Astronomy

S-MTT International Microwave Symposium Digest, 1974
A current review of recent observation of interstellar molecules in the millimeter wavelength region will be presented.
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Sub-Millimeter Astronomy and Astrophysics

1985
As of 1984, the submm band (ν >300 GHz) is relatively unexplored. The word “relatively” should be stressed since, evidently, a great deal of work has been done. However, much of this is of the “discovery” or “first detection” category with emphasis on the priority of a given result, and less thought as to astrophysical consequences.
T. L. Wilson, C. M. Walmsley
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MILLIMETER-WAVE OPTICS AND RADIO ASTRONOMY

Soviet Physics Uspekhi, 1962
Talk at the Physics Institute, Academy of Sciences U.S.S.R., at a meeting on March 12, 1962, commemorating the fiftieth anniversary of the death of P. N. Lebedev.
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7. clean energy
submillimeter astronomy
radio astronomy

protoplanetary disks
13. climate action
planet formation

science
fos: physical sciences
physics