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Träfflista för sökning "WFRF:(Strandberg Magnus 1975) srt2:(2010-2014)"

Sökning: WFRF:(Strandberg Magnus 1975) > (2010-2014)

  • Resultat 1-7 av 7
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2.
  • Belitsky, Victor, 1955, et al. (författare)
  • Design and performance of ALMA band 5 receiver cartridge
  • 2010
  • Ingår i: 35th International Conference on Infrared Millimeter and Terahertz Waves (IRMMW-THz), 2010. - 9781424466559 ; , s. 1-2
  • Konferensbidrag (refereegranskat)abstract
    • ALMA, Atacama Large Millimetre Array, covers the frequency band from 30 GHz to 960 GHz in ten separate frequency bands. We present here the design and performance of the ALMA Band 5 receiver cartridge that covers 163–211 GHz. The Band 5 receiver shows the state-of-the-art performance with the noise temperature below 65K (SSB) and sideband rejection above 12 dB over 80% of the RF band.
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4.
  • Billade, Bhushan, 1982, et al. (författare)
  • Performance of the First ALMA Band 5 Production Cartridge
  • 2012
  • Ingår i: IEEE Transactions on Terahertz Science and Technology. - 2156-342X .- 2156-3446. ; 2:2, s. 208-214
  • Tidskriftsartikel (refereegranskat)abstract
    • We present performance of the first ALMA Band 5 production cartridge, covering frequencies from 163 GHz to 211 GHz. ALMA Band 5 is a dual polarization, sideband separation (2SB) receiver based on all Niobium (Nb) Superconductor-Insulator-Superconductor (SIS) tunnel junction mixers, providing 16 GHz of instantaneous RF bandwidth for astronomy observations. The 2SB mixer for each polarization employs a quadrature configuration. The sideband separation occurs at the output of the IF hybrid that has integrated bias-T for biasing the mixers, and is produced using superconducting thin film technology.Experimental verification of the Band 5 cold cartridge performed together with warm cartridge assembly, confirms that the system noise temperature is below 45 K over most of the RF band, which is less than five photon noise (5 hf/k). This is to our knowledge, the best results reported at these frequencies. The measurement of the sideband rejection indicates that the sideband rejection better than 10 dB over 90% of the observational band.
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5.
  • Billade, Bhushan, 1982, et al. (författare)
  • Performance of the first ALMA Band 5 production cartridge
  • 2011
  • Ingår i: Proceedings of the 22nd International Symposium on Space Terahertz Technology, April 26-28th, 2011 - Tucson, Arizona, USA. ; , s. 56-56
  • Konferensbidrag (refereegranskat)abstract
    • We present performance of the first ALMA Band 5 production cartridge, covering RF frequencies from 163 GHz to 211 GHz. ALMA Band 5 is a dual polarization, sideband separation (2SB) receiver based on all Niobium (Nb) SuperconductorInsulator-Superconductor (SIS) tunnel junction mixer, providing 16 GHz of instantaneous RF bandwidth for the astronomy observations. The 2SB mixer for each polarization employs a quadrature layout. The sideband separation occurs at the output of the IF hybrid that has integrated bias-T for biasing the mixers, and is produced using superconducting thin film technology. Experimental verification of the Band 5 cold cartridge performed together with warm cartridge assembly, confirms the system noise temperature below 45 K, less than five quantum noise (5 hf/k) over most of the RF band, which is to our knowledge, the best results at these frequencies. The measurement of the sideband rejection indicates that the sideband rejection better than 10 dB over 90% of the observational band.
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6.
  • Nyström, Olle, 1979, et al. (författare)
  • Integrated Setup for THz Receiver Characterization
  • 2010
  • Ingår i: 21st International Symposium on Space Terahertz Technology 2010, ISSTT 2010; Oxford; United Kingdom; 23 March 2010 through 25 March 2010. - 9781617823626 ; , s. P6-4
  • Konferensbidrag (refereegranskat)abstract
    • A highly versatile measurement setup has been built that allows complete characterization of the ALMA Band 5 cartridge. The measurement setup includes all necessary hardware and largely achieves automatic measurements for the system noise and sideband rejection with in-built optimization procedures. The measurement setup additionally comprises measurements of the receiver saturation, phase and amplitude stability, as well as optical beam characterization.
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7.
  • Strandberg, Magnus, 1975 (författare)
  • Analysis, Simulation and Cryogenic/Mechanical Design for ALMA Band 5 Cartridge
  • 2011
  • Licentiatavhandling (övrigt vetenskapligt/konstnärligt)abstract
    • This licentiate thesis describes the work conducted by the author during the development of the ALMA Band 5 cartridge. The ALMA project as an international collaboration between various continents consisting of 66 antennas in total with ten ALMA receivers that observes in the range from 31 GHz and 950 GHz. The ALMA Band 5 receiver cartridge is designed for a frequency range of 163-211 GHz.For achieving the lowest possible system noise temperature, internal key components in the ALMA Band 5 cartridge, such as mixers and amplifiers, should experience a low temperature in the cryogenic region. By optimizing thermal heat load at various temperature stages and create a rigid structure by using various properties of material’s behaviour in cryogenic temperature, the cartridge are shown to be fulfilling all specified specifications.
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