Changes between Version 23 and Version 24 of Changes/atlod


Ignore:
Timestamp:
03/06/07 12:00:53 (17 years ago)
Author:
mci156
Comment:

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  • Changes/atlod

    v23 v24  
    1313
    1414== SYSCAL Record Changes ==
    15   The SYSCAL records will change from their current form.
     15 The SYSCAL records will change from their current form.
    1616
    17     SamplerStatistics::
    18       we no longer use these. So we need to avoid checking for them with CABB-type data.
     17 SamplerStatistics::
     18  we no longer use these. So we need to avoid checking for them with CABB-type data.
    1919
    20     StorageOfSYSCALData::
     20 StorageOfSYSCALData::
     21  Now that there are no sampler statistics, we need a different way of carrying along [wiki:Glossary/Tsys Tsys] and 
     22  [wiki:Glossary/XYPhase XYPhase] data than we have at present.
     23  At present there are 24 scalar values of Tsys (6 antennae * 2 polarizations * 2 IFs) written into every integration, and
     24  12 (6 ant. * 2 IFs) of XYPhase.[BR]
     25  [BR]
     26  In the new system there will likely be a spectrum of each, in the form of autocorrelations.
     27  Tsys is formed from the XX and YY polarisations of the autocorrelations, with the noise diode on and off;
     28  XYPhase from the XY (or its conjugate, YX) with the diode on and off.
    2129
    22      Now that there are no sampler statistics, we need a different way of carrying along [wiki:Glossary/Tsys Tsys] and 
    23      [wiki:Glossary/XYPhase XYPhase] data than we have at present.
    24      At present there are 24 scalar values of Tsys (6 antennae * 2 polarizations * 2 IFs) written into every integration, and
    25      12 (6 ant. * 2 IFs) of XYPhase.
     30  Deciding what to do here in terms of data representation requires discussions with WarwickWilson.
     31  Making changes here has flow on effects to other tasks that use Tsys or XYPhase.
    2632
    27      In the new system there will likely be a spectrum of each, in the form of autocorrelations.
    28      Tsys is formed from the XX and YY polarisations of the autocorrelations, with the noise diode on and off;
    29      XYPhase from the XY (or its conjugate, YX) with the diode on and off.
     33 ApplyingXYPhaseCorrections::
     34   At present atlod applies the XYPhase during filling. Nothing else (except maybe atxy) uses them.
     35   So we can compute the corrections, apply them and drop the XYPhase information, during ATLOD?
     36   May need to order the RPFITS data stream so that autocorrelations come before cross-correlations
     37   (and after SYSCAL records), so that the corrections for the cross-correlation can be computed
     38   before reaching the cross-correlations.
     39   We will need to carry Tsys info along but may be able to do it more compactly than storing the autocorrelations themselves.
    3040
    31      Deciding what to do here in terms of data representation requires discussions with WarwickWilson.
    32      Making changes here has flow on effects to other tasks that use Tsys or XYPhase.
    33 
    34     ApplyingXYPhaseCorrections::
    35       At present atlod applies the XYPhase during filling. Nothing else (except maybe atxy) uses them.
    36       So we can compute the corrections, apply them and drop the XYPhase information, during ATLOD?
    37       May need to order the RPFITS data stream so that autocorrelations come before cross-correlations
    38       (and after SYSCAL records), so that the corrections for the cross-correlation can be computed
    39       before reaching the cross-correlations.
    40       We will need to carry Tsys info along but may be able to do it more compactly than storing the autocorrelations themselves.
    41 
    42       Research required: The phase values computed on a per channel basis will be noisy, and applying them will just introduce noise.
    43       We need to understand how much smoothing across frequency will be needed.
    44       Need to do some experiments to understand the sequence of events in reading in a file.
     41   Research required: The phase values computed on a per channel basis will be noisy, and applying them will just introduce noise.
     42   We need to understand how much smoothing across frequency will be needed.
     43   Need to do some experiments to understand the sequence of events in reading in a file.
    4544
    4645 == DataSizeLimits ==