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. |
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. |
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. |