144 MHz Halo Antenna

Construction of a Low Cost Omnidirectional Horizontally Polarized Antenna for 144 MHz

by Dr. Carol F. Milazzo, KP4MD (posted 23 May 2012)
E-mail: kp4md@arrl.net


144
                    MHz Halo Antenna

1. Here is one of the pair of 2 meter Halo antennas I built this week. I needed a horizontally polarized antenna for a 144 MHz WSPR propagation study and planned to stack these to increase omnidirectional gain. I will use it with my Elecraft XV144 transverter with 20 watts peak output power and lower loss RG-8/U coaxial cable feed line. The materials for this one antenna cost about $6. Commercial versions cost about $50 or more.

144
                    MHz Halo Antenna

2. The boom is an 18 inch piece of the 1/2" Carlon "Plus 40" Rigid PVC Conduit that my husband had in the garden shed. I bought the 10 foot roll of 1/4 inch copper tubing for $9 at Home Depot. It comes coiled in nearly the required diameter. I cut a 41 inch length of it and easily formed it into the 13-1/8 inch diameter shape. The loop is continuous except for a gap between the open ends at the right end of the boom.

The
                    open ends of the loop here are separated by 1.5
                    inches. The resonant frequency of the antenna will
                    vary with the distance between these open ends. The
                    open ends of the boom will later be sealed for
                    weatherproofing.

3. The open ends of the loop here are separated by 1.5 inches. The resonant frequency of the antenna will vary with the distance between these open ends. The open ends of the boom will later be sealed for weatherproofing.

Detail of the 6-32 x 1" screw ready to be
                    soldered to the center pin of the SO-239 connector.

4. Detail of the 6-32 x 1" screw ready to be soldered to the center pin of the SO-239 connector.

144
                    MHz Halo Antenna

5. The 6-32 x 1" screw is soldered to the center pin of the SO-239 connector.

The
                    PVC Boom is drilled for the SO-239 antenna
                    connector. The center pin is 1-7/8" away from
                    the center point of the copper tubing.

6. The PVC Boom is drilled for the SO-239 antenna connector. The center pin is 1-7/8" away from the center point of the copper tubing.

Several #6 washers were placed under a #6 nut
                    to securely maintain its position and to prevent
                    traction on the solder joint when the mica trimmer
                    capacitor is secured onto the screw.

7. Several #6 washers were placed under a #6 nut to securely maintain its position and to prevent traction on the solder joint when the mica trimmer capacitor is secured onto the screw.

The
                    SO-239 antenna connector is secured to the PVC boom
                    with two 6-32 x 1½" screws.

8. The SO-239 antenna connector is secured to the PVC boom with two 6-32 x 1½" screws.

The
                    shell of the SO-239 connector is connected to the
                    copper tubing with 12 AWG bare copper wire which is
                    soldered to the tubing.

9. The shell of the SO-239 connector is connected to the copper tubing with 12 AWG bare copper wire which is soldered to the tubing.

The
                    side of the boom behind the SO-239 antenna connector
                    with the mica compression trimmer capacitor with a
                    6-32 nut onto the 6-32 screw that is soldered to the
                    center pin of the SO-239 connector.

10. The side of the boom behind the SO-239 antenna connector with the mica compression trimmer capacitor secured with a 6-32 nut onto the 6-32 screw that is soldered to the center pin of the SO-239 connector.

Close-up view of the mica compression trimmer
                    capacitor connected between the gamma match rod and
                    the screw on the center pin of the SO-239 antenna
                    connector.

11. Close-up view of the mica compression trimmer capacitor connected between the gamma match rod and the screw on the center pin of the SO-239 antenna connector.

I
                    investigated several feed methods and selected a
                    gamma match with a 30-180 pF mica compression
                    trimmer capacitor (Arco 463 type) soldered to a 6
                    inch length of the ¼" tubing. At maximum
                    capacitance, it barely brought the impedance 50 ohms
                    and zero reactance. The back-to-back alligator clips
                    are a temporary shorting bar.

12. I investigated several feed methods and selected a gamma match with a 30-180 pF mica compression trimmer capacitor (Arco 463 type) soldered to a 6 inch length of the ¼" tubing. At maximum capacitance, it barely brought the impedance 50 ohms and zero reactance. The back-to-back alligator clips are a temporary shorting bar.

The
                    original ¼

13. The original ¼" tubing gamma match arm was replaced with a 7" length of 10 AWG bare copper wire spaced 1-7/8" from the radiator element. This decreased the capacitance required to 80 pF to achieve the non-reactive 50 ohms impedance match. Tuning the antenna requires three adjustments: the gap space, the shorting bar location and the capacitor, and these all interact. With the capacitor at mid range, I first adjusted the gap for lowest SWR at 145 MHz, then adjusted the capacitor and moved the shorting bar position for lowest SWR. I repeated this procedure until finding the "sweet spot" where 1:1 SWR was achieved at 145 MHz and then soldered the shorting bar in place.

20
                    May 2012 - The 144 MHz halo antenna was mounted at
                    80 inches (1 λ) above the roof and fed with Belden
                    8214 foam type RG-8/U coaxial cable. At first, the
                    antenna resonance was unstable and sensitive to the
                    routing of the feed line until 5 turns of it were
                    wound to form a 8 inch diameter choke balun. The
                    standing wave ratio was then measured as 1:1 at
                    145.0 MHz.

14. 20 May 2012 - The 144 MHz halo antenna was mounted at 80 inches (1 λ) above the metal roof and fed with Belden 8214 foam type RG-8/U coaxial cable. At first, the antenna resonance was unstable and sensitive to the routing of the feed line until 5 turns of it were wound to form a 8 inch diameter choke balun. The standing wave ratio was then measured as 1:1 at 145.0 MHz.

A
                    closer view of the 144 MHz halo antenna. The entire
                    antenna was weatherproofed with clear acrylic spray
                    paint. The open ends of the boom and the PL-259
                    connector were sealed with a self sealing silicone
                    tape called Rescue Tape. Both open ends of the
                    copper loop were outside the boom with approximately
                    1.5" gap distance for resonance at 145 MHz.

15. A closer view of the 144 MHz halo antenna. The entire antenna was weatherproofed with clear acrylic spray paint. The open ends of the boom and the PL-259 connector were sealed with a self sealing silicone tape called Rescue Tape. Both open ends of the copper loop were outside the boom with approximately 1.5" gap distance for resonance at 145 MHz.

Close up view of the PL-259 antenna connector
                    sealed with Rescue Tape. The open spaces between the
                    boom and the SO-239 connector were sealed with GOOP
                    Plumbing contact adhesive and sealant, selected as
                    it does not release corrosive acetic acid during
                    curing.

16. Close up view of the PL-259 antenna connector sealed with Rescue Tape. The open spaces between the boom and the SO-239 connector were sealed with GOOP Plumbing contact adhesive and sealant, selected as it does not release corrosive acetic acid during curing.

144
                    MHz Halo antenna NEC model calculated SWR vs.
                    Frequency.

17. 144 MHz Halo antenna NEC model calculated SWR vs. Frequency.

144
                    MHz Halo antenna measured SWR vs. Frequency. The SWR
                    measured at the feed point was 1.3:1 or less over
                    the 144.0 to 146.4 MHz range.

18. 144 MHz Halo antenna measured SWR vs. Frequency. The SWR measured at the feed point was 1.3:1 or less over the 144.0 to 146.4 MHz range.

144
                    MHz Halo Antenna 4nec2 Calculations using the
                    high-pass L-network to simulate the gamma match.

19. 144 MHz Single Halo Antenna 4nec2 Calculations.  As the gamma match is not amenable to accurate NEC modeling1, I used the high-pass L-network under the RLC matching function (F10) of 4nec2 when generating the frequency sweep curves in Figures 17 and 20.

144
                    MHz Halo antenna NEC Model calculated Resistance and
                    Reactance vs. Frequency.

20. 144 MHz Halo antenna NEC Model calculated Resistance and Reactance vs. Frequency.

144
                    MHz Halo antenna measured Resistance and Reactance
                    vs. Frequency

21. 144 MHz Halo antenna measured Resistance and Reactance vs. Frequency.

144
                    MHz single Halo Antenna azimuth pattern calculated
                    by NEC Model.

22. 144 MHz single Halo Antenna azimuth pattern calculated by NEC Model.

144
                    MHz single Halo Antenna elevation pattern calculated
                    by NEC Model.

23. 144 MHz single Halo Antenna elevation pattern calculated by NEC Model.

144
                    MHz single Halo Antenna 3D Radiation Pattern
                    calculated by NEC Model.

24. 144 MHz single Halo antenna 3 dimensional radiation pattern calculated by NEC Model.

144
                    MHz 2 stacked Halo Antennas azimuth pattern
                    calculated by NEC Model.

25. 144 MHz 2 stacked Halo Antennas azimuth pattern calculated by NEC Model.

144
                    MHz 2 stacked Halo Antennas elevation pattern
                    calculated by NEC Model.

26. 144 MHz 2 stacked Halo Antennas elevation pattern calculated by NEC Model.

144
                    MHz 2 stacked Halo Antennas 3D Radiation Pattern
                    calculated by NEC Model.

27. 144 MHz 2 stacked Halo Antennas 3 dimensional radiation pattern calculated by NEC Model.

144MHz 2 stacked Halo Antennas 4nec2
                    Calculations.

28. 144 MHz 2 stacked Halo Antennas 4nec2 Calculations.

CM 144 MHz Halo Antenna NEC model by Carol F. Milazzo, KP4MD
CM Horizontal orientation (using GH command)
CM Frequency = 145.000 MHz
CM Impedance 50 ohms
CM 26-side polygon (40 inch loop with 1.5 inch gap)
CM Simulated good ground
CM Use the high-pass L-network to simulate the gamma match
CE
SY frq=145    'frequency MHz
SY cir=40.00758    'Input loop circumference inches (loop + gap)
SY r=0.5*cir/3.1415926    'Calculate loop radius
SY dia=0.25    'Input loop wire dia. inches
SY rad=0.5*dia    'Calculate loop wire radius
SY n=26    'Input n-side polygon of loop + gap
SY h=81.74    'Input height to loop inches
SY g=1.5    'Input gap size in inches
SY gseg=int(n*g/cir+0.5)    'Calculate gap length in segments
GH    1    n-gseg    1e-300    1e-300*(n-gseg)/n    r    r    r    r    rad
GM    0    0    0    0    gseg*180/n    0    0    h    0
GS    0    0    0.0254
GE    1
LD    5    0    0    0    58000000    '1/4 inch copper tubing
GN    2    0    0    0    4    0.01
EK
EX    0    1    (n-gseg)/2    0    1.    0    0    'Feed point
FR    0    0    0    0    frq    0
EN

29. 144 MHz Single Halo Antenna NEC model.

CM 144 MHz 2 Stacked Halo Antennas at 40 and 80 inches NEC model by Carol F. Milazzo, KP4MD
CM Horizontal orientation (using GH command)
CM Frequency = 145.000 MHz
CM Impedance 50 ohms
CM 26-side polygon (40 inch loop with 1.5 inch gap)
CM Simulated good ground
CE
SY frq=145    'frequency MHz
SY cir=40.21493    'Input loop circumference inches (loop + gap)
SY r=0.5*cir/3.1415926    'Calculate loop radius
SY dia=0.25    'Input loop wire dia. inches
SY rad=0.5*dia    'Calculate loop wire radius
SY n=26    'Input n-side polygon of loop + gap
SY h=81.74    'Input height to loop inches
SY g=1.5    'Input gap size in inches
SY gseg=int(n*g/cir+0.5)    'Calculate gap length in segments
GH    1    n-gseg    1e-300    1e-300*(n-gseg)/n    r    r    r    r    rad
GM    0    0    0    0    gseg*180/n    0    0    h/2    1
GM    1    1    0    0    0    0    0    h/2    1
GS    0    0    0.0254
GE    1
LD    5    0    0    0    58000000    '1/4 inch copper tubing
GN    2    0    0    0    4    0.01
EK
EX    0    1    (n-gseg)/2    0    0.5    0    0    'Feed point
EX    0    2    (n-gseg)/2    0    0.5    0    0    'Feed point
FR    0    0    0    0    frq    0
EN

30. 144 MHz 2 stacked Halo Antennas NEC model.

Two
                    identical 0.75 λ lengths of RG-11/U 75 ohm coaxial
                    cable were prepared for the stacking harness. After
                    trimming to achieve zero ohms reactance over 144 to
                    145 MHz, each of my cables measured exactly 40.25
                    inches from tip to tip. This measurement may vary
                    slightly due to variations in the velocity factors
                    among different batches and manufacturers of cable.

31. Two identical 0.75 λ lengths of RG-11/U 75 ohm coaxial cable were prepared for the stacking harness. After trimming to achieve zero ohms reactance at 145 MHz, each of my cables measured exactly 40.25 inches from tip to tip. This measurement may vary slightly due to variations in the velocity factors among different batches and manufacturers of cable.

The
                    two lengths of RG-11/U cable are joined with a UHF
                    Tee connector to form the stacking harness. When
                    measured from either end of the assembled stacking
                    harness, the SWR analyzer should indicate zero ohms
                    reactance and over 300 ohms resistance at 145 MHz.
                    When erected, the free end of each RG-11/U cable
                    will be connected to a halo antenna and the 50 ohm
                    feed line connected to the center of the Tee
                    connector.

32. The two lengths of RG-11/U cable are joined with a UHF Tee connector to form the stacking harness. When measured from either end of the assembled stacking harness, the SWR analyzer should indicate zero ohms reactance and over 300 ohms resistance at 145 MHz.  When erected, the free end of each RG-11/U cable will be connected to a halo antenna and the 50 ohm feed line connected to the center of the Tee connector.

The
                    lower halo is mounted at 40 inches height (0.5 λ)
                    above the roof and the upper halo is mounted 40
                    inches above it (1 λ). The gamma match sections
                    should be oriented on the same side of both halo
                    antennas.

33. The lower halo is mounted at 40 inches height (0.5 λ) above the roof and the upper halo is mounted 40 inches above it (1 λ). The gamma match sections should be oriented on the same side of both halo antennas.

A
                      weather shield was fashioned from a recyclable
                      plastic container and glued to the PVC boom of the
                      upper halo antenna. Its purpose is to protect the
                      feed point and the gamma match capacitor from
                      rain.

34. A weather shield was fashioned from a recyclable plastic container and glued to the PVC boom of the upper halo antenna. Its purpose is to protect the feed point and the gamma match capacitor from rain.

A
                      similar weather shield was placed on the lower
                      halo antenna. The spaces in and around the mating
                      surfaces of all the connectors were filled with
                      petroleum jelly and the connectors wrapped with
                      self-sealing silicone tape.

35. A similar weather shield was placed on the lower halo antenna.  The spaces in and around the mating surfaces of all the connectors were filled with petroleum jelly and the connectors wrapped with self-sealing silicone tape.

The red
                      line indicates the measured SWR for the stacked 2
                      meter halo antennas is less than 1.4:1 over the
                      144 through 146 MHz frequency range.

36. The red line indicates the measured SWR for the stacked 2 meter halo antennas is less than 1.4:1 over the 144 through 146 MHz frequency range.

NOTES ON HALO ANTENNA STACKING

  • Figure 30.  The separation distance of stacked halo antennas can be optimized for either gain or radiation pattern. Using my NEC model analysis, a 48 inch separation yielded 8.7 dBi gain at 15° elevation angle and a -8 dBi minor lobe at 90° elevation. The 40.5 inch separation yielded 7.9 dBi gain at 15° elevation and a -40 dBi sharp null at 90° elevation.  I selected the latter model to optimize the signal to noise ratio through both maximizing the gain in the desired direction while minimizing the gain toward noise sources from undesired directions.
  • Figure 31.  One method to determine the velocity factor of a coaxial cable is to attach one end of the cable to an antenna analyzer with the far end open, and to find the lowest frequency at which the measured impedance is zero. Then divide the cable length by the free space length of a quarter wave.  My RG-11/U coaxial cable's measured velocity factor was 0.66. I used this calculated velocity factor to cut each of my 75 ohm stacking harness sections to slightly longer than 3/4 wavelength at 145 MHz. With one end of each section attached to the antenna analyzer, I trimmed the far end until the analyzer read zero ohms reactance at the 145 MHz frequency with the PL-259 attached on both ends.  To account for the additional conductor length inside the Tee connector, the analyzer should read zero ohms reactance and over 300 ohms resistance when measuring from either end of the assembled stacking harness.  Fedler demonstrated an alternative method using an oscilloscope and function generator.8
  • Figure 33.  The proximity of each halo antenna to the other affects the tuning of both. With each of my halos mounted in its final location on the mast on the roof, I tuned each individually for minimal SWR at 145 MHz. When I then connected both of the antennas to the stacking harness, the SWR was 1:4 or lower from 144 MHz through 148 MHz (Figure 36) and no further adjustment was necessary.
  • Figure 33.  My RG-11/U stacking harness only allowed a single turn loop at the feed point of each halo, so my choke balun consisted of several turns of the 50 ohm coaxial cable at the Tee connector. The choke balun decouples the antenna from the feed line and stabilizes the tuning of the antenna that otherwise would be affected by any movement and the proximity of the feed line to other structures.

Radio
                      Mobile predicted line of sight signal strength for
                      stacked halo antennas at KP4MD station in Citrus
                      Heights, CA. Signal strength (0.004 µV) -30
                      dB to -20 dB SNR in orange area, greater than -20
                      dB SNR in yellow area. Transmitter power 50 watts,
                      antenna height 6 meters.

37. Radio Mobile Online predicted line of sight signal strength for stacked halo antennas at KP4MD station in Citrus Heights, CA. Limit of WSPR reception at signal strength (0.004 µV) -30 dB to -20 dB SNR in orange area, greater than -20 dB SNR in yellow area. Transmitter power 50 watts, antenna height 6 meters.

COMPARISON OF J-POLE VS. SINGLE AND STACKED HALO ANTENNAS

  • Figures 19 and 22 through 24 show the expected performance with a single halo antenna at 80 inches (1 λ) above the metal roof (effective ground).
  • Figures 25 through 28 and 39 through 41 show the expected performance with two stacked identical halo antennas, one at 40 inches (½ λ) and the other at 80 inches (1 λ) above the metal roof (effective ground).
  • Figures 42 through 44 show the predicted radiation patterns of the J-pole antenna.
  • The video clips at Figure 38 demonstrate the signal loss when antenna polarization is mismatched. 
  • The predicted increase in RDF (receiving directivity factor), the increased gain at 15º elevation and the suppression of the radiation lobes at 45º with the stacked halo antennas did improve the overall performance over the single halo antenna.

  • Test signal source - horizontally polarized beacon station KJ6KO/B on Bald Mountain, CA
  • Compared a vertically polarized J-pole antenna vs. the horizontally polarized single and dual stacked halo antennas
  • Arrow OSJ 146/440 J-pole antenna at 20 feet - Signal to noise ratio (SNR) = 23 dB
  • Single halo antenna at 18 feet with lobe oriented 90º away from KJ6KO/B - SNR = 38 dB
  • Two stacked halo antennas at 18 feet with lobe oriented 90º away from KJ6KO/B - SNR = 40 dB
  • Two stacked halo antennas at 18 feet with lobe oriented toward KJ6KO/B - SNR = 44 dB

38. Video clips comparing noise floor and received signals from KJ6KO/B on 144.283 MHz on Bald Mountain, CA.

144MHz 2 stacked Halo Antennas 3D Radiation
                    Patterncalculated by NEC Model.

39. 144 MHz 2 stacked Halo Antennas 3 dimensional radiation pattern calculated by NEC Model.  Composite of horizontal and vertical polarization components.

144
                    MHz 2 stacked Halo Antennas 3 dimensional radiation
                    pattern calculated by NEC Model. Horizontal
                    polarization component only.

40. 144 MHz 2 stacked Halo Antennas 3 dimensional radiation pattern calculated by NEC Model.  Horizontal polarization component only.

144
                    MHz 2 stacked Halo Antennas 3 dimensional radiation
                    pattern calculated by NEC Model. Vertical
                    polarization component only

41. 144 MHz 2 stacked Halo Antennas 3 dimensional radiation pattern calculated by NEC Model.  Vertical polarization component only.

144
                    MHz Arrow OSJ 146/440 J-Pole Antenna 3 dimensional
                    radiation pattern calculated by NEC Model

42. 144 MHz Arrow OSJ 146/440 J-Pole Antenna 3 dimensional radiation pattern calculated by NEC Model.  Composite of horizontal and vertical polarization components.

144
                    MHz Arrow OSJ 146/440 J-Pole Antenna 3 dimensional
                    radiation pattern calculated by NEC Model.
                    Horizontal polarization component only

43. 144 MHz Arrow OSJ 146/440 J-Pole Antenna 3 dimensional radiation pattern calculated by NEC Model.  Horizontal polarization component only.

144
                    MHz Arrow OSJ 146/440 J-Pole Antenna 3 dimensional
                    radiation pattern calculated by NEC Model. Vertical
                    polarization component only

44. 144 MHz Arrow OSJ 146/440 J-Pole Antenna 3 dimensional radiation pattern calculated by NEC Model.  Vertical polarization component only.

REFERENCES

  1. Some Preliminary Notes on the Gamma Match, Cebik, LB, W4RNL
  2. Horizontally Polarized Omni-Directional Antennas: Some Compact Choices, Cebik, LB, W4RNL
  3. Stacking 2 Meter Halo Antennas, Fedler M., N6TWW
  4. A Tree Friendly 2 Meter Halo Antenna, Krist, A., KR1ST
  5. Mobile 2-Meter 144 MHz SSB/CW "Halo", Merrill S., KB1DIG
  6. Stacking with Coax Cables as Transformation Lines, Steyer M., DK7ZB
  7. A 144 MHz Halo, Vallejo, Miguel A., EA4EOZ
  8. 2 Meter Halo Antenna Part 12 -- "Phasing Harness understanding & calculations", Fedler M., N6TWW
  9. 2 Meter Halo Antenna Project Video Series Parts 1-14, Fedler M, N6TWW

APPENDIX: NEC Model Files

  1. 144 MHz Halo Antenna NEC Model
  2. 144 MHz 2 Stacked Halo Antennas NEC Model
  3. 144 MHz 2 Stacked Turnstile Antennas NEC Model
  4. Arrow OSJ 146/440 J-Pole Antenna NEC Model

LINKS

  1. 144 MHz Halo Antenna Photo Album
  2. 144 MHz Halo Antenna Test Videos
  3. 144 MHz Omnidirectional Horizontal Antennas - NEC Model Comparisons of Stacked Halo, Turnstile and Eggbeater Omnidirectional Horizontally Polarized Antennas for 144 MHz
  4. Building the Elecraft XV Transverter Kit
  5. 144 MHz WSPR Propagation Study
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