VLBI at ALMA (MPIfR)

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    Version as of 15:44, 29 Mar 2024

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    This is the public page for our part of the "ALMA Phasing Project" (APP) at MPIfR.

    If you are looking for the "official" APP pages go here.

    The APP project was presented By W. Alef at the "11th European VLBI Network Symposium & Users Meeting"

    The presentation can be found here, the proceedings will soon become available here.

    Summary of the APP project

    By phasing all ALMA dishes together into a single effective aperture, ALMA can operate as both an exceptionally sensitive mm/sub-mm VLBI element and a beamformed array suitable for high frequency pulsar work. A detailed design for implementing a system to phase up the array has been completed and funding to build and integrate this capability into ALMA has been secured. With this system in place, ALMA will become a key element in Global mm/sub-mm VLBI arrays that target a broad range of high sensitivity and high angular resolution science.

    APP status

    The APP has passed both the preliminary design review and the critical design review and is being implemented.

    First tests are planned for early 2014, the project will end with the commissioning pf the phasing system early 2015.

    Overview

    alma_phasing_blk_diag_rev16-1.pngALMA phasing block diagram. The red boxes exist, the blue boxes have to be added for phasing ALMA, and the green colour groups boxes into larger units. (for details see attached paper)

    alma_phasing_sw_rev5-1.png


     

     

     

     

     

     

     

    Modifications needed for ALMA software. The red boxes exist, the blue boxes have to be added for phasing ALMA, and the green colour groups boxes into larger units. (for details see attached paper)