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Millimeter Radio Astronomy and the Solar Convection Zone
PLANETARY RADIO EMISSIONS VII, 2011The global distribution of solar surface activity (active regions) is connected with processes in the convection zone. To extract the information on large-scale motions in the convection zone, we study the solar synoptic charts (Mount Wilson 1998-2004, Fe I, 525.02 nm). The clear indication of large-scale (= 18°) turbulence is found.
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New Directions for Millimeter Astronomy in the 21st Century
1994To advance beyond the impressive achievements of the current generation of mm and sub-mm elescopes, an obvious step for astrophysics in the 21st century is construction of an array with ten times the collecting area of existing mm telescopes. This means ~ 10000 m2, equivalent to the collecting area of the Effelsberg 100 m telescope or the VLA, but ...
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Design considerations for a multibeam receiver for millimeter wave astronomy
International Journal of Infrared and Millimeter Waves, 1987A progress report was given for a multibeam system with only a limited (3–4) number of beams. We have outlined the desirability of larger arrays and some instrumental consquences were considered. We have also shown that extension of the JCMT infrastructure could fulfil the requirements but most of the development need to be done in the frontend segment.
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Millimeter-Wave Receivers and Their Applications in Radio Astronomy (Short Papers)
IEEE Transactions on Microwave Theory and Techniques, 1974T G Phillips
exaly
Low-noise heterodyne receivers for near-millimeter-wave radio astronomy
Proceedings of the IEEE, 1985J W Archer
exaly
Aluminum LEKIDs for millimeter-wave radio astronomy
2014 39th International Conference on Infrared, Millimeter, and Terahertz waves (IRMMW-THz), 2014Glenn Jones +11 more
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