RadioAstron Closed Loop for DiFX

    Version as of 21:35, 29 Apr 2024

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    Introduction

    RadioAstron has two modes of synchronization: 1) local synchronization with a H-maser reference and an on-board rubidium reference, and 2) "closed-loop" with synchronization using the H-maser references at Pushchino and Greenbank ground stations.

    The H-maser reference was depleted in July 2017. This left the rubidium as the only on-board reference.

    Astro Space Center (ASC) reports in RadioAstron Newsletter #33 that the synchronization mode with the on-board reference produced interferometric fringes, but best results were achieved in the closed-loop mode. 

    Closed-loop mode of synchronization is the default for AO5 and AO6 observations.

    The ASC has a dedicated software correlator for RadioAstron experiments. The ASC correlator already implements a delay model that incorporates closed-loop mode.

    The DiFX software correlator supports space VLBI ("RA-DiFX"). It too is used for correlating RadioAstron experiments. However, currently RA-DiFX does not support the closed-loop mode (01/2019).

    Source code location

    This page keeps track of implementing closed-loop support into the existing DiFX RadioAstron source code branch.

    The current not yet modified RA-DiFX source code resides in https://svn.atnf.csiro.au/difx/master_tags/DiFX-RA-1.0.0/ and is installed in /cluster/difx/DiFX-RA-1.0.0/, selectable on the cluster with 'dra100'.

    Updates

    22Nov2018 : brief exchange with J. Anderson (RA-DiFX) on patching closed-loop delays into DiFX CALC model .im files

    17Dec2018 : test data set RK18CJ received at Bonn, no documentation

    07Jan2018 : first look at raw data and .vex; created v2d and vex.obs; ground-only, no fringes yet (Irbene/Yebes/Noto)

    Test data set

    Data are on the cluster under /data/rk18cj/ and /Exps2/rk18cj/

    Raw data

    /data/rk18cj/rdf/GBTS_20172920*.rdf RadioAstron raw 4-channel 1-bit data in RDF(?) format
    /data/rk18cj/ra/GBTS_20172920*.m5b RadioAstron raw RDF converted to raw Mark5B
    /data/rk18cj/gb/NRAO+312_005?_RK18CJ_GB_No000? GBT, 4-thread 1-channel 2-bit VDIF
    /data/rk18cj/{ys,mc,ir,nt}/* Yebes and others stations, 1-thread 4-channel 2-bit VDIF
    /data/rk18cj/tr/* Torun, unknown format

    Extra files

    README "This is a RadioAstron experiment raks18cj to test the RadioAstron correlation for the closed-loop (coherent mode) observations."
    filelist_RA_v2d.txt spacecraft / ground station clock breaks in undocumented notation
    rdf/GBTS_2017_292_rk18cj.txt RDF file 1-bit statistics in 4-channels for all four scans
    RA_C_COH.TXT RadioAstron delay polynomials for each scan
    RA_C_COH_uvw.txt RadioAstron polynomials for u, v, and w

    Missing information:

    1. reference FITS visibility data set, to be able to compare ASC results against DiFX
    2. clocks and rates used for the ground stations in the ASC reference correlation
    3. EOPs used in the ASC reference correlation
    4. details on the polynomials; is RA_C_COH.TXT in seconds, does it include ground-to-space delay?

    Correlation details

    Details of DiFX correlation are below.

     

    Station Format Delay Rate Notes
    Noto @6cm VDIF/8032 fs log "gps-fmout/-48.48e-06" ? none yet
    Yebes @6cm VDIF/8032 ? ? none yet
    Irbene @6cm VDIF/8032 ? ? none yet
    RadioAstron @6cm Mark5B-128-4-1 ? ? none yet
    GBT @1.3cm (automatic) ? ? none yet
    Medicina @1.3cm VDIF/8032 ? ? none yet
    Torun @1.3cm --unknown-- fs log, no gps-fmout ? none yet

    Delay polynomial

    Details on implementation in DiFX