EVLA Memo # 194 EVLA Ka-band Receiver Down Converter Module Harmonics: The Mega-Birdie at MHz

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EVLA Memo # 194 EVLA Ka-band Receiver Down Converter Module Harmonics: The Mega-Birdie at 29440 MHz R. Selina, E. Momjian, W. Grammer, J. Jackson NRAO February 5, 2016 Abstract Observations carried out using the Ka-band receivers of the EVLA show an extremely strong spectral feature (a birdie) at 29440 MHz. This frequency is the 230 th harmonic of 128 MHz, and the 2 nd harmonic of the L301-1 synthesizer. Our investigation shows that this feature is due to the leakage of the fundamental Local Oscillator (LO) frequency into the Intermediate Frequency (IF) of the Ka-band receiver block Down Converter Module (DCM). Reducing this LO leakage into the IF will require an expensive redesign of the DCM. 1. Introduction This report is the conclusion of an investigation into the source of the 29440 MHz birdie. The frequency 29440 MHz is the 230th harmonic of 128 MHz, and the birdie is visible on all baselines and cross correlation products. The spectrum in Figure 1 from the RFI spectral sweep shows the birdie prominently. The spectrum is a scalar average of all the baselines in the D-configuration of the array in RR, and has a channel separation of 125 khz. Hanning smoothing was applied. The scale is logarithmic (in db) with an arbitrary offset. The birdie is also seen in the LL correlation. Figure 1: The 29440 MHz birdie. The spectrum is a scalar average of all the baselines in the D-configuration in RR. The scale is logarithmic, in db, with an arbitrary offset. 1

2. Summary of Findings The 29440 MHz birdie is the 2nd harmonic of 14720 MHz, which is the default (auto) tuning of the L301-1 1 for Ka-band observations centered at 34.5 GHz and below. 2 The RFI sweep script uses the automatic system tuning, and therefore would be tuned as such for the lower portion of the Ka-band utilizing the Intermediate Frequency (IF) pair B/D. The harmonic is due to leakage of the fundamental Local Oscillator (LO) frequency into the IF path of the Ka-band receiver block Down Converter Module (DCM). When the fundamental LO is present in the IF, it will appear to the user as the second fundamental of the LO in the Radio Frequency (RF). Based on laboratory tests of EVLA Ka-band DCM Serial Number (S/N) 32, the LO leakage power is -73dBm in to the IF. This is unfortunately the tuning with the worst rejection of the fundamental LO within the Ka-band DCM tuning range. Other legal tuning values have LO rejection of 80-100dB or more. The results are summarized in Table 1. The fundamental LO is shown in the first column. The leaked LO power in to the IF is shown in column 2. The second and third harmonic frequencies are shown in columns three and four, respectively. The range of the legal tunings for the Ka-band receiver s down converter is highlighted, with band edges shown in orange. See Table 2 for the full results. f LO P LO IF (dbm) f 2 x LO f 3 x LO 13952 < -100 27904 41856 14208 < -100 28416 42624 14464-80 28928 43392 14720-73 29440 44160 14976-95 29952 44928 15232 < -100 30464 45696 15488 < -100 30976 46464 15744-80 31488 47232 16000 < -100 32000 48000 16256-96 32512 48768 16512-93 33024 49536 16768 < -100 33536 50304 Table 1: The leaked LO power in to the IF in the Ka-band Down Converter Module Serial Number 32. The highlighted fields denote the range of the legal tunings for the Ka-band down converter, with band edges shown in orange. The Ka-band DCM is built around a Monolithic Microwave Integrated Circuit (MMIC) which is not easily modified. Reducing LO leakage into the IF would require a redesign of this module, at significant expense in both dollars and manpower that is not recommended at this time. Should a user have a spectral line or other features they wish to investigate in the vicinity of this spur, the spur can be moved to other frequencies shown in the third column of Table 1. E.g., tuning the fundamental LO to 14976 MHz would both reduce the amplitude of the spur and move it to 29952 MHz. A permanent 1 The L301-1 is the synthesizer that is used for the Ka-band block down conversion. 2 Tuning parameters were computed using the Tuning Auto program ( Test Auto Config of EVLA ) available on the SSS Test Programs page: Http://builder.aoc.nrao.edu/sssTestPgm.shtml 2

change in tuning would move the lower frequency limit for the IF pair AC from 32 GHz to 32.76 GHz. Since this is a feature advertised to users, a policy decision would be required. 2.1. Future Installations Should the EVLA Ka-band receiver be installed at the VLBA or other sites, it is unlikely that the DCM would be reworked and/or redesigned to eliminate this spur. As an integrated MMIC module, any changes would involve prototyping and testing that is currently inconsistent with the crashed schedules proposed for the VLBA Ka-band upgrade. 3. Investigated Hypotheses Three possible ways this harmonic may be coupled into the signal path were identified and investigated: 1) Present at the output of the L301-1, and inadequately attenuated by existing filters in the LO path. 2) Present at the output of the L301-1, and radiated from the L301-1 and associated coaxial cables into the Ka-band feed. 3) Generated as a mixer product, or by a device in the LO path, of the Ka-band block Down Converter Module (DCM). 4. On-Antenna Tests Tests were performed on antenna ea01 on May 7, 2015. A maintenance script was run to setup the antenna for Ka-band, the LO tuning was adjusted to the bandpass of interest, and the bandpass was plotted to confirm the presence of the 29440 MHz birdie (see Figure 2). A second, stronger birdie, at roughly 29480 MHz is also visible in the total power data. This feature may have also been seen in the RFI sweeps, but it is much weaker compared to the 29440 MHz birdie (see Figure 3). The tuning of the L301-1 was changed to both 14464 MHz and 14976 MHz (the L301 is tuned in 256 MHz increments) to determine if the birdie moves with tuning. As expected, the birdie moves to 28928 MHz and 29952 MHz, respectively. A follow up observation was performed on May 12, 2015. A sequence of four figures (Figure 4 Figure 7) shows the birdie moving from 29400 MHz to 29952 MHz when the L301-1 is tuned to 14720 MHz and 14976 MHz, respectively. We note that the birdie previously seen at 29480 MHz is no longer visible in this observation. Conclusion: The 29440 MHz birdie appears in the spectrum as the second harmonic of the L301-1. However, how this harmonic is coupled into the signal path is unclear. 3

Figure 2: Bandpass plot using the default tuning from the Ka-band maintenance script. The observation was carried out on 2015-05-07. The 29440 MHz birdie (marked) is the weaker of the two visible in this plot. The 29480 MHz birdie may have been present during the RFI spectral sweep as can be seen in Figure 3. Figure 3: A spectrum at K-band from the RFI sweep showing weaker birdies. The 29480 MHz birdie (marked) may only be present in the RR polarization product. 4

Figure 4: Follow up observation on 2015-05-12. The birdie is at 29440 MHz with the default L301-1 tuning. Figure 5: The birdie at 29440 MHz is not present once the fundamental LO, from the L301-1, is tuned away from 14720 MHz. 5

Figure 6: No birdie at 29952 MHz with the L301-1 tuned to 14720 MHz. Figure 7: The birdie at 29952 MHz when the L301-1 is tuned to 14976 MHz. 6

5. L301-1 Characterization The output level of the L301-1 was tested in the lab to determine the power of the second harmonic of the LO. Measurements are typically given in dbm with dbc in parenthesis. The L301-1 was set up with a short (~3 ft) section of heliax cable and no DC block to the input of an Agilent-8565 50 GHz spectrum analyzer. The L301-1 was tuned to 14720 MHz for the duration of the test. The 2 nd harmonic of the output (29440 MHz) has an output power of -72dBm (-83.5dBc). Other birdies are visible at odd multiples of 128 MHz: 29568 MHz (231 st harmonic of 128 MHz), -66.8dBm (-78.3dBc). 29824 MHz (233 rd harmonic of 128 MHz), -83.7dBm (-95.2dBc). 30080 MHz (235 th harmonic of 128 MHz), -74.8dBm (-86.3dBc). Note that the 512 MHz comb and its harmonics are not visible on the spectrum analyzer. Output power at 14848 MHz, the nearest comb line, was -86dBm (-97.5dBc), while at 29696 MHz it is below the noise level of the spectrum analyzer. The power of these harmonics (with the marginal exception of 29568 MHz) meets the specifications for the L301-1. The specification, from the EVLA project book, is as follows: Output Power: +11dBm (Nominal and Adjustable) Output Spurious signal level: <-70 dbc (Except for harmonics of Ref (i.e., the 128 MHz reference) Output harmonics of Ref: <-80 dbc The 128 MHz harmonics appear to be intermodulation products. Their composition is given by (2 x nearest comb) + (N x 128 MHz). It is worth noting that the 231 st, 233 rd and 235 th harmonics of 128 MHz are not present in the RFI spectral sweeps. Conclusion: The 2 nd harmonic of the output is not the highest power harmonic, and none of the nearby harmonics of comparable power are visible in the RFI spectral sweep data, therefore the L301-1 is not likely to be the cause of the 29440 MHz birdie visible in the IF. There are also long coaxial cables, with high attenuation above 18 GHz, and filters within the IF path of the Ka-band receiver DCM, therefore the amplitudes of these spurs would be significantly attenuated before the block down converter mixer. 6. Ka-band Receiver LO Path The frequency trippler in the LO path of the Ka-band receiver may be producing a second or a fourth harmonic of the fundamental LO supplied by the L301-1. A block diagram of the receiver can be seen in Figure 8. Laboratory testing of EVLA Ka-band DCM S/N 32 confirms that that there is leakage of the fundamental LO into the IF port from the block down converter. When the fundamental LO is tuned to the default 14720 MHz, the LO leakage power is -73dBm in to the IF. Test results are summarized in Table 1 and the full test results are shown Table 2. The 128 MHz input to the L301-1 is used as a digital reference within the module, so it is clipped to a square wave. This may also be generating the additional harmonics, but is less likely than mixer products. 7

F309 - Ka-Band (26-40 GHz ) Front End Ka Band Feed Ka Band PS OMT Tnoise=20K +35 +35 Noise NF=5dB +15 +15 +10 44.0-49.0 GHz X3 X3 44.0-49.0 GHz +10 L -47 dbm/ghz -36 dbm/14 GHz Ka-BAND LO from L301-1 via S7/S8 R COOLED Tnoise=20K NF=5dB Power: 50W, (allow 1.2A @ 54.2 VDC) Figure 8: VLA Ka-Band Receiver Bock Diagram. Configuration of the DCM module is diagrammatic only. Actual schematic differs. Due to the arithmetic of the down conversion process, when the fundamental LO is present in the IF, it will appear to the user as the second fundamental of the LO in the RF. Unfortunately, the LO tuning of 14720 MHz has the worst rejection of the fundamental LO within the Ka-band DCM tuning range. Other legal tuning values have LO rejection of 80-100dB or more. The Ka-band DCM is an integrated MMIC module that is not easily modified. Reducing LO leakage into the IF would require a redesign of this module, at significant expense in both dollars and manpower. 8

f LO P LO IF VMIX (dbm) (V) f 2 x LO f 3 x LO f 4 x LO f 5 x LO f 6 x LO f 7 x LO f 8 x LO f 9 x LO 5248-80 2.510 10496 15744 20992 26240 31488 36736 41984 47232 5504-53 2.510 11008 16512 22016 27520 33024 38528 44032 49536 5760-77 2.506 11520 17280 23040 28800 34560 40320 46080 51840 6016-86 2.512 12032 18048 24064 30080 36096 42112 48128 54144 6272-45 2.510 12544 18816 25088 31360 37632 43904 50176 56448 6528-73 2.503 13056 19584 26112 32640 39168 45696 52224 58752 6784-90 2.493 13568 20352 27136 33920 40704 47488 54272 61056 7040-87 2.511 14080 21120 28160 35200 42240 49280 56320 63360 7296-56 2.512 14592 21888 29184 36480 43776 51072 58368 65664 7552-69 2.505 15104 22656 30208 37760 45312 52864 60416 67968 8064-86 2.506 16128 24192 32256 40320 48384 56448 64512 72576 8320-86 2.511 16640 24960 33280 41600 49920 58240 66560 74880 8832-79 2.490 17664 26496 35328 44160 52992 61824 70656 79488 9088-96 2.433 18176 27264 36352 45440 54528 63616 72704 81792 9344-98 2.447 18688 28032 37376 46720 56064 65408 74752 84096 9600-65 2.478 19200 28800 38400 48000 57600 67200 76800 86400 9856-43 2.420 19712 29568 39424 49280 59136 68992 78848 88704 10112-70 2.433 20224 30336 40448 50560 60672 70784 80896 91008 10368-81 2.360 20736 31104 41472 51840 62208 72576 82944 93312 10624-71 2.392 21248 31872 42496 53120 63744 74368 84992 95616 10880 < -100 2.406 21760 32640 43520 54400 65280 76160 87040 97920 11136 < -100 2.364 22272 33408 44544 55680 66816 77952 89088 100224 11392 < -100 2.297 22784 34176 45568 56960 68352 79744 91136 102528 11648 < -100 2.343 23296 34944 46592 58240 69888 81536 93184 104832 11904 < -100 2.257 23808 35712 47616 59520 71424 83328 95232 107136 12160-85 2.219 24320 36480 48640 60800 72960 85120 97280 109440 12416-98 2.289 24832 37248 49664 62080 74496 86912 99328 111744 12672 < -100 2.513 25344 38016 50688 63360 76032 88704 101376 114048 12928 < -100 2.513 25856 38784 51712 64640 77568 90496 103424 116352 13184 < -100 2.513 26368 39552 52736 65920 79104 92288 105472 118656 13440 < -100 2.513 26880 40320 53760 67200 80640 94080 107520 120960 13696 < -100 2.513 27392 41088 54784 68480 82176 95872 109568 123264 13952 < -100 2.503 27904 41856 55808 69760 83712 97664 111616 125568 14208 < -100 2.502 28416 42624 56832 71040 85248 99456 113664 127872 14464-80 2.510 28928 43392 57856 72320 86784 101248 115712 130176 14720-73 2.377 29440 44160 58880 73600 88320 103040 117760 132480 14976-95 2.308 29952 44928 59904 74880 89856 104832 119808 134784 15232 < -100 2.219 30464 45696 60928 76160 91392 106624 121856 137088 15488 < -100 2.153 30976 46464 61952 77440 92928 108416 123904 139392 15744-80 2.137 31488 47232 62976 78720 94464 110208 125952 141696 16000 < -100 2.196 32000 48000 64000 80000 96000 112000 128000 144000 16256-96 2.110 32512 48768 65024 81280 97536 113792 130048 146304 16512-93 2.084 33024 49536 66048 82560 99072 115584 132096 148608 16768 < -100 2.488 33536 50304 67072 83840 100608 117376 134144 150912 17024 < -100 2.509 34048 51072 68096 85120 102144 119168 136192 153216 17280 < -100 2.513 34560 51840 69120 86400 103680 120960 138240 155520 17536 < -100 2.513 35072 52608 70144 87680 105216 122752 140288 157824 17792-99 2.513 35584 53376 71168 88960 106752 124544 142336 160128 18048-98 2.513 36096 54144 72192 90240 108288 126336 144384 162432 18304-94 2.513 36608 54912 73216 91520 109824 128128 146432 164736 18560 < -100 2.513 37120 55680 74240 92800 111360 129920 148480 167040 Table 2: Ka-band DCM LO leakage tests using the receiver S/N 32 with effective LO Leakage to IF output from (n x f LO - (n-1) x f LO ). Legal LO tunings are highlighted in the red rectangle. 9