A side-band-separating (SBS) heterodyne mixer has been designed for the Atacama Large Millimeter Array (ALMA) 602-720 GHz band, as it will present a great improvement over the current double-side-band configuration under development at the moment. Here we present design details and the results of extensive computer simulations of its performance. The designed SBS mixer exploits waveguide technology. At its core it consists of a quadrature hybrid, two LO injectors, and three dumping loads. The entire structure has been analyzed in a linear circuit simulator with custom code written to accurately (verified by HFSS finite element simulations) model the hybrid structures. This technique permitted an optimization of the dimensions and the study ...
We presented the design and experimental results of a new sideband-separating (2SB) mixer for 600-72...
We presented the design and experimental results of a new sideband-separating (2SB) mixer for 600-72...
The ALMA band 9 (600-720 GHz) receiver cartridge, as currently being produced, features two single-e...
A side-band-separating (SBS) heterodyne mixer has been designed for the Atacama Large Millimeter Arr...
In this article we present the design, modeling and construction of a side-band-separating (2SB) het...
Here we present the realization of a side-band-separating (2SB) heterodyne mixer for the frequency r...
The Atacama Large Millimeter Array (ALMA) is the largest radio astronomical enterprise ever proposed...
This licentiate is focused on the design and development of Superconductor-Insulator-Superconductor ...
We designed, built and tested a new sidebandseparating mixer assembly for the 600-720 GHz band (ALMA...
For high-frequency observational bands like ALMA (Atacama Large Millimeter Array) Band 9 (600—720 GH...
The Atacama Large Millimeter Array (ALMA) is the largest radio astronomical enterprise ever proposed...
We presented the design and experimental results of a new sideband-separating (2SB) mixer for 600-72...
We presented the design and experimental results of a new sideband-separating (2SB) mixer for 600-72...
The ALMA band 9 (600-720 GHz) receiver cartridge, as currently being produced, features two single-e...
A side-band-separating (SBS) heterodyne mixer has been designed for the Atacama Large Millimeter Arr...
In this article we present the design, modeling and construction of a side-band-separating (2SB) het...
Here we present the realization of a side-band-separating (2SB) heterodyne mixer for the frequency r...
The Atacama Large Millimeter Array (ALMA) is the largest radio astronomical enterprise ever proposed...
This licentiate is focused on the design and development of Superconductor-Insulator-Superconductor ...
We designed, built and tested a new sidebandseparating mixer assembly for the 600-720 GHz band (ALMA...
For high-frequency observational bands like ALMA (Atacama Large Millimeter Array) Band 9 (600—720 GH...
The Atacama Large Millimeter Array (ALMA) is the largest radio astronomical enterprise ever proposed...
We presented the design and experimental results of a new sideband-separating (2SB) mixer for 600-72...
We presented the design and experimental results of a new sideband-separating (2SB) mixer for 600-72...
The ALMA band 9 (600-720 GHz) receiver cartridge, as currently being produced, features two single-e...