The WAPP (Wideband Arecibo Pulsar Processor, as this device first
reached astronomers as a pulsar processor, with standard spectral-line
operation appearing later), is the replacement for the ``interim''
correlator. The WAPP provides eight sub-correlators,
each of these sub-correlators having sixteen 1024-lag chips.
Each of 4 pairs of sub-correlators
can be set up with their own independent bandwidths
and configurations. Table 5 specifies the available
configurations. The maximum bandwidth per sub-correlator is 100 MHz,
with 9 other alternative bandwidths being available in decreasing
octave steps. The WAPP offers both 3- and 9-level operation, both for
standard autocorrelation (total-power) and auto+cross correlation (all
four Stokes parameters) modes. The WAPP also offers a direct-sampling
option. Details of the many WAPP capabilities are to be found at
http://alfa.naic.edu/hardware/backend/wapp_fact_sheet.html, with
the WAPP 8-board mode
being described at http://www.naic.edu/~cima/cima_dual_board.html.
| Config | Max Bw | Pol/Sbc |
Lags/Sbc |
| per Sbc |
(kms@ 1420 MHz) |
||
| Single-Pixel 100-MHz Bandwidth | |||
| 9-level | 100 | 1 | 2048 (2.6) |
| 9-level | 100 | 2 | 1024 (5.2) |
| 3-level | 100 | 1 | 8192 (2.6) |
| 3-level | 100 | 2 | 4096 (2.6) |
| 3-level Stokes | 100 | Full Stokes | 2048 (2.6) |
| Single-Pixel 195-kHz - 50-MHz Bandwidth | |||
| 9-level | 50 | 1 | 4096 (2.6) |
| 9-level | 50 | 2 | 2048 (5.2) |
| 3-level | 50 | 1 | 16384 (2.6) |
| 3-level | 50 | 2 | 8192 (2.6) |
| 9-level Stokes | 50 | Full Stokes | 2048 (2.6) |
| 3-level Stokes | 50 | Full Stokes | 8192 (2.6) |
| ALFA 100-MHz Bandwidth | |||
| 3-level | 100 | 2 | 4096 (2.6) |
| 3-level Stokes | 100 | Full Stokes | 2048 (2.6) |
| ALFA 50-MHz Bandwidth | |||
| 9-level | 50 | 2 | 2048 (5.2) |
| 3-level | 50 | 2 | 8192 (2.6) |
| 9-level Stokes | 50 | Full Stokes | 1024 (2.6) |
| 3-level Stokes | 50 | Full Stokes | 4096 (2.6) |