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The Side Band Filter

The Side Band Filter



The Dual Beam Interferometer (DBI)

RxB3 has a dual beam (Mach-Zehnder) interferometer that permits single or double sideband observations. The DBI has two movable arms, though in practice the necessary path differences are achieved by moving only one arm (number 1) under computer control. The normal operating position as shown on the PF2 Display screen of arm 2 is 9.0. Unlike many of the adjustable receiver parameters that are stored in look-up tables as functions of frequency, the arm position is calculated for each tuning.

Side Band Rejection

When tuned in SSB mode, the image side band lines are typically reduced in intensity by about 13dB (i.e. a factor of ~ 20). Thus strong lines in the blocked sideband may still appear weakly in the spectrum. Also, because the transmission properties of the DBI are not quite flat across the passband, there may be a small variation in this rejection ratio across the wider spectral windows.

LO Power

When tuned in DSB mode the interferometer transmits both the LO frequency and the side band frequencies unimpeded. However, in SSb the image band is blocked and the transmission at the LO frequency is 50%. Consequently, when the DBI is optimally tuned for DSB operation, the LO power to the mixers is maximized. In SSB mode at the same frequency it is halved. Generally this is not of importance but it is useful to keep mind if you're tuning to an extreme frequency where LO power is at a premium. (But also remember that, especially at the high frequency end, the atmosphere is relatively opaque and SSB mode will generally produce significantly lower system temperatures.)


Contact: Ming Zhu. Updated: Thu Dec 30 14:36:24 HST 2004

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