A comprehensive engineering analysis of RFI mitigation strategies, ferrite core selection, noise reduction techniques, and signal-to-noise ratio improvements for the Collins 51S-1 series receivers. Covers nine modification intercept points across the signal chain, power supply, and oscillator subsystems. The 51S-1 was designed by Ed Andrade, W0DAN (SK) in collaboration with Gene Senti, W0ROW and remains one of the finest general-coverage tube receivers ever produced.[1]
collinsradio.org/archives/manuals/Collins51S-Receiver.pdf
Full-size 11×17 fold-out reproductions with professional comb binding are also available from ke9pq.com. The CCA equipment page for the 51S-1, maintained with contributions from Rod Blocksome, K0DAS, Larry Saletzki, WA9VRH, and Charlie Talbot, K3ICH, is the definitive online resource.[3]
Architecture Overview
The 51S-1 is a dual- or triple-conversion communications receiver covering 0.2–30.0 MHz in thirty 1-MHz bands.[4] Triple conversion is used for the 0.2–7.0 MHz range, and double conversion for 7.0–30.0 MHz. The final IF is 500 kHz; selectivity in SSB and CW modes is provided by Collins mechanical filters. A Q-multiplier is fitted for additional interference rejection. Sensitivity for SSB/CW above 2 MHz is specified at 0.6 µV for 10 dB S+N/N.
The receiver originated in a hallway conversation between Chuck Carney, W0GDJ (SK, then Collins marketing manager), Gene Senti, W0ROW, and Ed Andrade, W0DAN, who remarked that the 51J-4 was “getting a little long in the tooth” and they could “do better.”[5] Jerry Vonderheide, W0NGL served as production engineer when the design was transferred to production, and later created the 51S-1A (28 VDC aircraft version). Over 12,360 units were manufactured between 1961 and 1982, the highest production quantity of any 51J-series receiver.[6]
Modification Points — Engineering Analysis
Nine intercept points are identified across the signal chain and power subsystem. Each is described with the circuit location, noise mechanism, and a practical implementation using current ferrite materials. Ferrite mix selection follows the guidance of Tom Rauch, W8JI and the Fair-Rite Products Corporation published material specifications.[7]
The single largest source of RFI ingress in any vintage receiver is conducted common-mode noise riding on the coax shield from the antenna feedline. The 51S-1 antenna input is 50 Ω unbalanced at J1,[4] with the signal immediately entering impedance-matching transformer L30. A toroid-wound common-mode choke installed at J1, before L30, stops conducted RF from the shack environment — SMPS hash, LED driver noise, PC USB interference — from entering the receiver while passing the differential antenna signal with negligible insertion loss.
ImplementationWind 8–10 turns of RG-316 (or equivalent small-diameter coax) through a Fair-Rite Type 31 toroid (p/n 2631801202, 1.4″ OD). Type 31 (MnZn, μ ≈ 1500) provides 400–1000 Ω of common-mode impedance across 1–30 MHz.[8] For MW and low-band work below 2 MHz, substitute Type 75 or Type 77 mix for better low-frequency permeability. A split ferrite clamp (Fair-Rite 0431164281) at the antenna entry provides additional suppression without rewiring.
The RF amplifier following the double-tuned input network (L33/L32/L31, C40, L69/L68/L67, C71, turret wafers A1–A5) sets the noise figure for the entire receiver. The tuning slugs of L32 and L68 are mechanically ganged to the main tuning control.[4] Factory screen bypass capacitors on V1 are often marginal by current standards, and supply lead inductance allows HF hash to reach the screen grid directly, raising the receiver noise floor.
ImplementationAdd a Fair-Rite Type 43 ferrite bead (100 Ω at 100 MHz, p/n 2643000201) on the screen grid B+ lead immediately adjacent to the socket pin, followed by a 0.01 µF / 630 V ceramic disc cap to chassis. Repeat on the plate load resistor B+ lead. Type 43 (NiZn, μ ≈ 850) provides suppression from 10 MHz upward — the range where IF strip spurious responses and oscillator harmonics radiate into the front end.[9] Do not use Type 61 or Type 67 here; those mixes are optimised above 50 MHz and provide insufficient impedance at HF.
The IF strip contains the mechanical filter, AGC-controlled IF amplifiers, the Q-multiplier, and the product detector — all sharing a common B+ bus. Ripple and high-frequency hash on this bus modulates IF gain stages and raises the noise floor, particularly on weak SSB signals. The first local and first line AF amplifiers obtain input signal from either the SSB/CW preamplifier Q1, or from AM detector CR15, selected by the EMISSION switch S2.[10] The original wax-and-paper bypass capacitors are almost certainly deteriorated; replacement alone provides measurable noise floor improvement.
ImplementationOn each IF stage B+ feed, add a Fair-Rite Type 43 ferrite bead (1/4″ lead, 600 Ω at 25 MHz) immediately at the tube socket B+ pin, followed by a 0.1 µF / 630 V film cap (Vishay MKP or equivalent) to chassis. Replace all original wax-and-paper bypass capacitors. For mechanically filtered stages, add a 10 Ω / 2 W carbon film resistor in series with the B+ feed to each IF transformer primary to form a passive RC decoupling section.
The BFO (V15) generates the product detector injection signal at approximately 500 kHz. Poorly bypassed BFO B+ leads allow 500 kHz injection signal to couple into the audio chain, producing a low-level heterodyne tone particularly audible on SSB with AGC released. Microphonics from a loose BFO circuit can masquerade as broadband noise. The BFO coupling capacitor to the product detector should be a high-stability silver-mica or C0G ceramic type if previously serviced with a ceramic disc replacement.[11]
ImplementationWrap the BFO compartment with 3M 1181 copper foil tape, bonded to chassis with conductive adhesive or a solder lug. Add Fair-Rite Type 43 beads on V15 plate and screen leads. Ensure V15 has a snug tube shield with firm contact on its retaining ring. Verify the BFO coupling capacitor is silver-mica or C0G; replace if a standard ceramic disc type is found.
Output transformer T4 uses negative feedback to V14A cathode to reduce line amplifier distortion.[10] The 600 Ω balanced line output is inherently well protected, but the local speaker/headphone output is an unbalanced path that acts as an antenna for conducted RFI. RF rectification in semiconductor junctions in connected external equipment can feed noise back into the audio chain through the headphone jack — a mechanism well documented by W8JI and others.[7]
ImplementationOn the local audio output, fit a small common-mode choke wound on a Fair-Rite 2643625702 (Type 43, 0.5″ OD dual-hole balun core), 5–6 bifilar turns. Add 0.01 µF / 50 V C0G caps from each audio lead to chassis after the choke. Add 100 Ω series resistors at the phones jack to prevent RF rectification. For the 600 Ω balanced line output, verify the TB1 transformer centre-tap ground solder joint is solid; a cracked joint is a common source of hum on this series.[12]
The 51S-1 draws approximately 125 watts from the AC line with a conventional mains transformer. The 50–400 Hz power frequency specification reflects the receiver’s original military and aviation heritage, where power quality is highly variable.[4] Modern shack environments deliver an AC line rich in switching noise from LED drivers, variable-speed motor controllers, and switching power supplies — all sources entirely absent when the 51S-1 was designed in 1960.
ImplementationInstall a commercial AC line filter (Schaffner FN2010-6-06 or equivalent 6 A / 250 V EMI filter) at the power entry point, or construct an equivalent using X2 differential capacitors (0.1 µF) and a common-mode inductor wound on a Fair-Rite Type 31 toroid (200 µH, 3 A). Bond the filter case directly to the 51S-1 chassis with a short braided strap. Physically separate the filtered and unfiltered power leads inside the chassis.[8]
The Collins 70K-7 permeability-tuned oscillator operates on a regulated low-voltage supply. Any ripple or transient on this supply causes the characteristic frequency hopping reported in community discussions.[13] Phase noise on the PTO directly determines the receiver’s reciprocal mixing performance on strong adjacent signals. Diodes CR501 (series) and CR502 (Zener) are the first suspects in any frequency instability complaint. The 70K-7 uses a permeability-tuned coil mechanism; the core slug must be clean and the coil form crack-free.
ImplementationReplace CR501 with a 1N4148 and CR502 with a 1N5230B or BZX79C5V1 Zener if either tests soft or leaky. Add a 10 µF / 35 V low-ESR electrolytic cap directly across the PTO B+ supply close to the tube socket. For maximum stability, add a further RC filter — 10 Ω in series, 47 µF across the output — ahead of the existing Zener regulation. This mod is consistent with the diagnostic approach documented in the EDAboard 51S-1 community forum.[13]
The 51S-1 perforated wrap-around cabinet increases ground impedance compared to a solid-steel chassis. At audio frequencies, multiple return current paths form loops that intercept magnetic flux from the power transformer, manifesting as 60 Hz and 120 Hz hum. Green oxidation on aluminium chassis lugs is common on receivers of this era and adds measurable impedance. A restoration by Grayson Evans (WN4GVM/now KJ7UM) documents this as a first-priority maintenance item on the 51S-1.[14]
ImplementationIdentify the chassis point physically closest to the power transformer secondary centre tap and designate it the star ground. Run a braided copper strap (minimum 3/4″ wide, as short as physically possible) from the audio ground bus to this star point. Tie the RF ground bus in the front-end area to the star point via a separate short, wide braid — not through the perforated chassis. Torque all original chassis lug screws and clean oxidised contact surfaces with IPA before reassembly.
The high-frequency crystal oscillator V2B operates on all bands; frequency is determined by one of sixteen crystals on the turret wafer selected by the MEGACYCLES control. The 17.5 MHz oscillator V3B operates only for the 2–7 MHz range. Radiation from these oscillators into the RF stages produces internal birdies. In the 0.2–2.0 MHz range, the 51S-1 instruction book itself notes internally generated spurious whistles at 333 kHz, 666 kHz, 1000 kHz, 1500 kHz, and 2000 kHz.[2]
ImplementationWrap the turret assembly perimeter with 3M 1181 copper foil tape, ensuring shield continuity across all joints. Bond the foil to the turret frame with silver conductive epoxy or a machine screw through a solder lug. Add individual Fair-Rite Type 43 ferrite beads on V2B and V3B plate and grid leads at the tube sockets. Do not add beads on the crystals themselves — the crystal series resistance interacts with the load and can shift frequency or cause oscillation instability.[9]
Additional SNR Improvement — 55G-1 Preselector
Ferrite Material Selection Summary
Ferrite mix selection follows Fair-Rite published material data and the amateur radio community guidance of Tom Rauch, W8JI and Gene Hinkle, K5PA.[7][15]
| Location | Fair-Rite Mix | Typical Part | Reason |
|---|---|---|---|
Coax antenna entry common-mode choke |
Type 31 |
2631801202 (1.4″ OD toroid) |
MnZn, μ≈1500 • broadband HF, 1–300 MHz CM suppression |
Tube B+ leads, screen grids (IF strip, RF amp) |
Type 43 |
2643000201 (0.25″ bead) |
NiZn, μ≈850 • 10–300 MHz, high loss, VHF suppression |
AC mains common-mode choke |
Type 31 |
2631803802 or equivalent 3 A rated |
MnZn • low-frequency hash, 100 kHz–30 MHz |
Audio output common-mode choke |
Type 31 / 77 |
2643625702 dual-hole balun core |
MnZn • LF through lower HF; audio CM suppression |
Toroidal inductors for RC decoupling filters |
Type 52 / 61 |
Various, per inductance required |
NiZn • stable inductance, low loss, suited to wound inductors |
Key rule: Type 43 is the workhorse bead for individual tube lead bypassing (NiZn, effective at HF and above). Type 31 is the broadband HF common-mode suppressor for antennas, power leads, and signal lines (MnZn, best below 30 MHz). Never substitute Type 61 beads on B+ leads in the IF strip — Type 61 is optimised above 50 MHz and provides almost no suppression at the HF frequencies where IF strip noise coupling occurs.[8]
Recommended Implementation Priority
Work from the environment inward. Address power supply and ground noise first, then antenna-conducted RFI, then tube-level refinements. The 51S-1 — designed by Ed Andrade, W0DAN with its specified spurious responses at not less than 70 dB down above 2 MHz[4] — is an exceptionally well-engineered receiver. Most of its noise limitations in a modern shack arise from the environment, not from deficiencies in the original 1960 design.
- Mod F — AC Line Filter: Eliminates conducted noise injected into the receiver from the mains. The highest-impact single modification in a modern shack environment.
- Mod H — Star Ground: Eliminates ground loop hum at 60/120 Hz. Should be performed alongside Mod F as part of the same session.
- Mod A — Coax Entry Choke: Stops antenna-conducted RFI from entering the receiver at J1 before any amplification occurs. Type 31 toroid; 8–10 turns of RG-316.
- Mod G — PTO Stabilisation: Address immediately if frequency hopping is observed. CR501/CR502 replacement is a quick diagnostic step before deeper investigation.[13]
- Mod C — IF Strip Decoupling: Replace all wax-and-paper bypass caps; add ferrite beads and RC decoupling on B+ feeds. Significant noise floor improvement on SSB.
- Mod B — V1 Screen Bypass: Improves receiver noise figure; particularly beneficial above 14 MHz where atmospheric noise falls below the receiver noise floor.
- Mod I — Turret Oscillator Shielding: Reduces internal birdies, most audible on the 0.2–2.0 MHz bands.
- Mod D — BFO Shielding: Eliminates residual heterodyne tone on SSB; worth doing as part of a complete IF strip service.
- Mod E — Audio Output Filter: Last priority; primarily benefits headphone operation and long cable runs to external equipment.
Credits & Acknowledgements
Lead designer, 51S-1 / 51J-4 / R-390 / KWM-2. Passed away 24 August 2007, Satellite Beach, Florida.
Collins engineer; developed the 51S-1 conversion scheme and birdie chart.
Collins marketing manager; co-initiated the 51S-1 concept conversation with W0DAN and W0ROW.
Collins engineer on Ed Andrade’s 51S-1 team; later succeeded Gene Senti as engineering group leader.
Key Collins lab technician; completed the first lab models of the 51S-1 in 1960.
Collins production engineer; created the 51S-1A (28 VDC aircraft variant) and oversaw production transfer.
Collins engineer; contributed prototype documentation including the machined-brass tuning knob history.
Rockwell Collins engineer (42+ yrs); author of the definitive 51S-1 HF Receiver CCA feature article, production surveys, and Collins historical research. ARRL Midwest Division Vice Director.
Edited the CCA 51S-1 product document; CCA contributor and Collins community historian.
CCA contributor to the 51S-1 equipment page and production data research.
CCA contributor to the 51S-1 equipment page and variant documentation.
Widely cited technical expertise on ferrite bead selection, RFI suppression, and split-core bead verification using the MFJ-259B. See eham.net ferrite article.
Author of the Fair-Rite Clamp-on Core Selection Guide, widely used in the amateur community for ferrite mix identification and application.
Maintained the wa3key.com 51S-1 Receiver page, an important secondary resource for circuit description and operational notes.
The CCA (collinsradio.org) is the primary archive for all Collins Radio manuals, service bulletins, and technical history. An invaluable community resource.