Radio telescope receivers for ALMA
Daniels Electronics has successfully completed a $1.3 million contract with the Canadian government for the assembly and test of radio receivers used in the National Research Council of Canada (NRC) development of 84-116 GHz heterodyne receivers for the international Atacama Large Millimeter Array (ALMA) telescopes.
ALMA is located at 5000 m elevation in the Chajnantor Plain of northern Chile. The resolution and sensitivity of the array will provide a leap forward, making it a pre-eminent radioastronomy facility.
NRC’s contribution to the project included 73 extremely sensitive 84-116 GHz receivers. The nucleus of the receiver is a superconductor-insulator-superconductor (SIS) tunnel mixer which downconverts the RF signal collected by the radio telescope to an intermediate frequency (IF) signal centred at 6 GHz with a bandwidth of 4 GHz.
A cryogenic high electron mobility transistor (HEMT) amplifier is used to amplify the IF signal by more than 30 dB before it is delivered to the ALMA back-end system. The SIS detector and the HEMT IF amplifier must operate at a cryogenic temperature of 4 Kelvin. NRC has developed a cryogenic 4-8 GHz HEMT amplifier for this application.
CASA issues 40,000th remote pilot licence
In recent years, remote (drone) pilots have overtaken CASA-licensed fixed-wing aircraft,...
Comms Connect draws international headliners to Melbourne
The 19th edition of Comms Connect Melbourne will feature the largest number of international...
Motorola Solutions completes Silvus Technologies acquisition
Motorola Solutions plans to extend Silvus's reach through its global scale and longstanding...