Each unit can be placed in the [100,600] MHz IF band, in steps of 0.625MHz
(by using a third frequency conversion). The 40, 80 and 160MHz bandwidths
are synthesized by the adjacent upper and lower sidebands of an image
rejection mixer. Low-pass filters select the desired bandwidth. Note that
these bandwidths show the Gibbs phenomenon right in the middle of the band
(i.e. at the edges of the IRM sidebands). The central two channels are
flagged by default, the observer should avoid to place the most important
part of the line there. The 10 and 20MHz bandwidths do not
have this restriction: for the 20MHz bandwidth, only the upper sideband
of the IRM is used. The 10MHz bandwidth (only unit 5) is produced by slowing
down the clock rate from 40 to 20MHz.
The spectroscopic capabilities of the cross-correlator at Plateau de
Bure are summarized in Table 4.5. Part of the flexibility
is achieved by using the ``time-multiplexing'' technique. For example,
a time-multiplexing factor four means that the data, arriving at a rate of
samples/s, are alternately put into four shift-registers.
The shift registers are read out at the clock frequency of 40MHz, thus
creating four data streams taken at a rate that is lower by a factor of four
(as compared to the sampling speed). Equivalently, a time-multiplex factor two
means two data streams at a rate of 80MHz each.
Bandwidth | Sideband | Clock | Time | Number | Complex | Channel | Spectral | |
of IRM(1) | Rate | Multiplex | of Lags | Channels | Spacing | Resolution | ||
Factor | (2) | [MHz] | (3) | (4) | ||||
160 | USB + LSB | 40 | 4 | 64 | 64 | 2.500 | 3.025 | 4.000 |
80 | USB + LSB | 40 | 4 | 128 | 128 | 0.625 | 0.756 | 1.000 |
40 | USB + LSB | 40 | 2 | 256 | 256 | 0.156 | 0.189 | 0.250 |
20 | USB | 40 | 2 | 512 | 256 | 0.078 | 0.094 | 0.125 |
10 | USB | 20 | 1 | 512 | 256 | 0.039 | 0.047 | 0.062 |