Zobrazeno 1 - 10
of 39
pro vyhledávání: '"Arto Lehto"'
Autor:
Antti V. Räisänen, Arto Lehto, Urban Frisk, Jussi Tuovinen, T. Hirvonen, Juha Ala-Laurinaho, P. Piironen
Publikováno v:
IEEE Transactions on Antennas and Propagation. 49:1264-1270
Development work of a 119 GHz compact antenna test range (CATR), based on a 2.4 m/spl times/2.0 m hologram and its application on the Odin telescope tests are described. The hologram element comprises seven parts, which are fabricated using silk-scre
Publikováno v:
IEEE Transactions on Antennas and Propagation. 47:1125-1130
A low-profile high-gain antenna array of box horns for the frequency band 57.2-58.2 GHz is presented. The antenna consists of 256 radiating elements divided into two subgroups of 128 elements fed by a rectangular waveguide feed network. The radiating
Publikováno v:
IEEE Transactions on Antennas and Propagation. 46:1189-1193
A planar antenna in which box horns are used as radiating elements is described. The feed network is built by connecting rectangular waveguides with T-junctions. The matching of the T-junctions is improved by using rounded splitters and matching pins
Publikováno v:
International Journal of Infrared and Millimeter Waves. 17:807-818
A planar single-ended GaAs Schottky diode mixer has been designed, built, and tested at 119 GHz. The mixer front end includes also a waveguide filter for image rejection, and a temperature compensated ring filter. Measurements at room temperature sho
Publikováno v:
Microwave and Optical Technology Letters. 28:396-398
Publikováno v:
Experimental Astronomy. 2:149-161
The spectral line receiving system at the 13.7 m radio telescope at the Metsahovi Radio Research Station is described. A cooled low noise Schottky mixer receiver in 72–115 GHz range is employed. The back end system comprises three acousto-optical s
Publikováno v:
Scopus-Elsevier
A cooled receiver having a DSB noise temperature of 80-140 K in the frequency range 75-95 GHz has been built for radio astronomical observations. The quasioptical beam switch is followed by a 3 mm Schottky mixer and FET amplifier at 1.4 GHz. A phase
Autor:
S.N. Dudorov, Arto Lehto, Ville Viikari, Juha Mallat, V.S. Mottonen, Juha Ala-Laurinaho, Antti V. Räisänen, Dmitri Lioubtchenko, Janne Häkli, Tomi Koskinen, Anne Lönnqvist
Publikováno v:
Ala-Laurinaho, J, Mallat, J, Häkli, J, Koskinen, T, Lönnqvist, A, Viikari, V, Mottonen, V, Dudorov, S, Lioubtchenko, D, Lehto, A & Raisanen, A V 2005, Millimetre wave antenna research at Helsinki University of Technology . in ANTEM 2005 : 11th International Symposium on Antenna Technology and Applied Electromagnetics, Conference Proceedings ., 7852017, IEEE Institute of Electrical and Electronic Engineers, 11th International Symposium on Antenna Technology and Applied Electromagnetics, ANTEM 2005, Saint-Malo, France, 15/06/05 . https://doi.org/10.1109/ANTEM.2005.7852017
Aalto University
Aalto University
This paper describes the research work at the Radio Laboratory of Helsinki University of Technology concerning millimetre and submillimetre wave antenna technology: development of new antenna designs and, especially, development of antenna measuremen
Publikováno v:
IEEE Antennas and Propagation Society International Symposium. 1999 Digest. Held in conjunction with: USNC/URSI National Radio Science Meeting (Cat. No.99CH37010).
A planar array of box horns is presented for the frequency band 57.2-58.2 GHz. The horns are fed in parallel with a waveguide feed network. Improved T-junctions are used to connect the waveguides. The horns are divided into two subarrays shifted side
Publikováno v:
IEEE Antennas and Propagation Society International Symposium. 1999 Digest. Held in conjunction with: USNC/URSI National Radio Science Meeting (Cat. No.99CH37010).
This paper presents a simple broadband dual-polarized microstrip antenna with only three layers. The input impedance bandwidth (VSWR 40 dB) between the ports and thus acceptable cross polarization (better than -20 dB). The geometry, return loss, and