Calibration of loop antennas at VLF - NIST Page is suggested by Greene ... calc~ll?-ted by...

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JOURNAL OF RESEARCH of the National Bureau of Sta nda rds-C. Engineering and Instrumentation Vol. 65, No.3, Ju ly-September 1961 Calibration of Loop Antennas at VLF 1 A. G. Jean, H. E. Taggart, and 1. R. Wait (Febr uary 21, 1961) A tec hniqu e a nd the equi pment used for the precise d etermin at ion of fi eld stren gt h of signals received from VLF t ra nsmi tters is des cribed. The e quipm ent, whi ch is b atte ry- op erated, con tains provisions for t he recept io n of VLF signals and the gen erat ion of stand ar d fi elds to an ac curac y of 5 percent. Both the receivin g" nd tra nsmitt in g a nt e n ll as ar e loops. Th e fi eld st rengt h is d etermin ed in te rms of a qu asi-s tat ic magnetic fi el d wi t h t he t wo loo p antenn as positioned co axia ll y at a spacing of a pprox im ately two met ers. Al th ough the te chniqu e was dev eloped f or use 9t VL F, it ca n be used at higher frequencies for ca lib rat ing loop ante nna s, generato rs, a nd volt mete rs, a nd f or d ete rmining eff ect ive heights of a nt ennas, or simil a r a pplica t ions. 1. Introduction , iVi th the in creased use of the very low frequ en cy portion of the radio spec trum , an ur gent need exi sts for th e accur ate calibra tion of receiving ant enn as opera ting in t hi s frequ en cy range. Conven tion al met hods of calibr at ing loop an tenn as requir e th at th ey be pl aced in a radi ation fi e ld . In other word s, the separ ation b et v leen th e test sour ce and the receiving antenn a is large compared to th e wave- len gth. At VLF this requir ement becomes imprac- ti cal; for exampl e, the wavelen gth at 10 kc/s i 30 km . A test sour ce placed at di stances greater than this m ay require several kilowa tts of power to pro- vide a signal th at will comp ete with th e atmo pheri c noise level. It is suggested by Gr eene [19 5 1] th at a free space ra diation field could be simul ate d adequ ately at the receiving antenn a if the test source were also a loop an tenn a and placed coaxially with, and close to , th e receiving loop ant enn a which is to be calibrated. Th e magni t ud e of the equivale nt radi ation fi eld at the receiving loop antenn a is then calcula ted in terms of the geome try and configuration of the two loop s. Such an equation has been s tated by Greene [1951] without proof. It is the purpose of t his paper to invet;tigate th e general applicability of Greene's equation, to outline a techniqu e used for the pr ecise and accurate deter- min ation of fi eld streng th using this equation , and finally to describe the equipment used to perform these measurements . 2. Theoretical Basis The necessary equ a tions for calibrating a loop receivin g ant enn a with a coaxial test tran smi t ting loop ar e first considered. The di stance of separation is arbi trary, and the dimensions of the loops are ass umed small compar ed to th e wavelen gth. The situ at ion is illus trat ed in fi gur e l. 1 Cont l"ib ution fro m Central R adio Propagation Laboratory and Radio Stand- ards Laboratory, National Bureau of Standards, Boulder, Colo. d FIGU RE 1. Si mplified view of t wo coaxi al loops. Th e ac tu al valu e of the v olt age v indu ced in receiving loop m ay be expressed in te rms of the max- imum eq ui valen t electric fi eld , E" th at would exist in a free-space radi at ion fi e ld . The relationship for an electrically small loop is simpl y 271" where f3 = "}:, (1) but v= IZ"" where Z ,n is the mu tual imp edance between the loops. Where all dimensions are elec- trically small and curr ent s in the loop are constant , we have exactly j J.LW (1'1)1. [ ( F) ] Z",= ( 271"1'z ) 7I"k r; 2 1- 2 K (k)- E (k) (2) =. ) J J.LW 16 1'2 4 128 . . . , (3) [ 41' 11'2 J! d d wh er e k= (1'1 + 1'2 )2 + d2 an 1 '1 an 1' 2 are the trans- mit ting a nd receiving loop radii, r es pectively, a nd d is th eir cent er-to-center separ ation. K (k) a nd E (k ) are elliptic in tegrals as tabulated by Dwight r1947]. Th e above e qu ation for Z ", may be obtained from a numb er of differen t S OUTces, including Smythe [1950] who gives a formula for th e <p- component of th e 593949- 61- 5 189 J

Transcript of Calibration of loop antennas at VLF - NIST Page is suggested by Greene ... calc~ll?-ted by...

Page 1: Calibration of loop antennas at VLF - NIST Page is suggested by Greene ... calc~ll?-ted by integrating E",= -jwA", around the ... Calibration of loop antennas at VLF ...

JOURNAL OF RESEARCH of the National Bureau of Sta ndards-C. Engineering and Instrumentation Vol. 65, No.3, July-September 1961

Calibration of Loop Antennas at VLF 1

A. G. Jean, H. E. Taggart, and 1. R. Wait

(February 21, 1961)

A technique a nd t he eq uipment used for t he precise determination of field s t rength of signals received from VLF t ra nsmitters is described . The equipm ent , which is battery­operated , con tains provisions for t he recep t ion of VLF signa ls a nd t he generation of standard fields to a n accuracy of 5 percent. Bot h t he receiving" nd transmit t in g a nt en ll as are loops. The fi eld st rength is determined in terms of a quasi-stat ic ma gn etic fi eld wi t h t he t wo loop antenn as posit ioned coaxia lly at a spacing of approximately two meters . Al t hough t h e technique was developed for use 9t VLF , i t ca n be used at high er freq uencies for calibratin g loo p a nt ennas, generators, and volt meters, a nd for determin ing effective h eights of a ntenn as, or s imila r a pplica t ions.

1. Introduction

, iVith the increased use of the very low frequency portion of the radio spectrum, an urgen t need exists for the accura te calibra tion of receiving antennas opera ting in t his frequency range . Conven tion al methods of calibrating loop an tennas require t hat they be placed in a radiation field . In other words, the separation betvleen the test source and the receiving an tenna is large compared to the wave­length . At VLF this requirement becomes imprac­tical ; for example, t he wavelength at 10 kc/s i 30 km . A tes t source placed a t distances greater than this may require several kilowatts of power to pro­vide a signal that will compete with the atmo pheric noise level.

It is sugges ted by Greene [1951] that a free space radiation field could be simulated adequately at the receiving an tenna if the t est source were also a loop antenna and placed coaxially with, and close to , the receiving loop antenna which is to be calibrated. The magnitude of the equivalent radiation field a t the receiving loop antenna is then calculated in terms of the geometry and configuration of the two loops. Such an equation has been stated by Greene [1951] without proof.

It is the purpose of t his paper to invet;tiga te the gen eral applicability of Greene's equation, to outline a technique used for the precise and accurate deter­mination of field strength using this equation, and finally to describe the equipment used to perform these measurements.

2 . Theoretical Basis

The necessary equations for calibrating a loop receiving antenna wi th a coaxial test transmit ting loop are first considered . The distance of separation is arbitrary, and the dimensions of the loops are assumed small compared to the wavelength . The situation is illustrated in figure l.

1 Contl"ibution from Cen tral R adio P ropagation Laboratory and R adio Stand­ards Laboratory, N ational Bureau of Standards, Boulder , Colo.

d

FIGU RE 1. S i mplified view of two coaxial loops.

The ac tual value of the voltage v induced in th~ receiving loop may be expressed in terms of the max­imum eq ui valen t electric field, E" that would exist in a free-space radiation field. The rela tionship for an electrically small loop is simply

271" wher e f3= "}:, (1)

but v= IZ"" where Z,n is the mutual impedance between the loops. Where all dimensions are elec­trically small and currents in the loop are constant, we have exac tly

j J.LW (1'1)1. [ ( F) ] Z",= (271"1'z) 7I"k r; 2 1- 2 K (k)- E (k) (2)

= . 7I"1'2 (~)!Xk3 (1+~ k2+~ k4+ ) J J.LW 16 1'2 4 128 . . . ,

(3)

[ 41'11'2 J! d d where k= (1'1 + 1'2)2+ d2 an 1'1 an 1'2 are th e trans-

mitting and receiving loop radii, r espectively, and d is their center-to-cen ter separation. K (k) and E (k) ar e ellip tic in tegrals as tabula ted by Dwight r1947]. The above equation for Z", may be obtained from a number of differen t SOUTces, including Smyth e [1950] who gives a formula for the <p-component of the

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vector potential, A"" of a loop carrying a constant current I. The mutual impedance Zm is then calc~ll?-ted by integrating E",= -jwA", around the recmvmg loop. The length of this path is 27r1'2.

Thus,

E '" 607rr2 I [ 3 2 75 4 J f w + (1'1 + r2)2]3/2X 1+ 4: k + 128 k + .. .. (4)

Neglecting terms in the series above k2 it is seen that this expression can be reduced as foliows

3 1'1' (1' 1')2 1+4: lc2 ",1 + 3Tz+tenns in Tz w + (1'1 + 1'2)2]3/2 (d2+ 1'i+ 1'~+ 21'I1'2p/ 2

'" 1 X[l+ " (1'I1'2)2J = W + 1'i+ 1'W/2 terms m (j2 . (5)

The last expression is the denominator in Greene 's equation [1951] . If ?oth ~oops have radii compa­ra~le to d, th~ quantIty k ]s not small compared to umty, and hIgher terms must be retained in the series . At higher frequencies where dlA cannot be neglected compared to unity, a correction factor may be applied which is the ratio of the coaxial magnetic field of a small loop at wavelenath A to the infinite wavelength case. This is lul~wn to be 1 +.i27rdIA and has a magni tude

as stated by. qTeene [19~1 ]. It is strictly valid for d> > 1'1, but It ]s only a mmor second order correction at medium frequencies and is completely negligible at VLF.

Equation (4) is va~id for d etermining the equiva­lent free-space electn c field s trength if 1'1 , 1'2, and d are electn cally small compared to A. Since this eq.ua tion is ~trictlJ~ valid. only in free-space, the effect~ of nmghbonng obJects have been verified e~penmentally b~- moving m etallic objects of various sI~es near the loop antennas and observing the 6ffects on the system. If the near est sizable objects are separated from the loops by approximately two to thre~ tImes the loop spacmg, el, the resulting error wIll be less than abou t 1 percent. The m eas­urements should not be performed in a shielded ~oom, and the measurement site should be free of farge metallic objects such as overhead power lines :-II' similar objects.

3. Calibration Procedure

Two basic method s are applicable to the measure­.nent of fi eld intensity [IRE Standards 1942]' one . h ' , IS t e standard-antenna method , and the other is the standard-field method. In th e former a standard l'eceivi~g. antenna is use~ so that the voltage pro­~uced m It by a field of gIven intensity and polariza­~lOn m ay be comput~d . The usual voltage m easured IS not th e open-circUlt antenna voltage but is related

to it through a voltage transfer ratio. It is some­t~es difficylt to determine this voltage transfer ratlO to a hIgh degree of accuracy.

In the stand ard-field method , a standard field is set up by a local transmitting arrangement, and the field at. the recmvmg antenna is computed from the dimenSlOns of the receiving and transmitting an­tennas, the separation distance between the antennas, and the current in the transmitting loop . In this technique the equipment consists of a suitable receiver equipped with a m eter to indicate the rela­tive strength of the r eceived fi eld. The strenath of the .r eceived field is determined by compariI~g the recmver output voltage produced by the field under measuremen t with the voltage produced by a stand­ard fi eld. Eac~ of the basic methods offers certain advantages

and dIsadvantages dependent upon the applica tion . In the case under consideration , the standard-field method was adopted because of the straio'htforward ca~ibration method which can be evolved using co­aXIal loop antenna arrangmnents as discussed above.

The calibration equipment is represented in figure 2; that to the left is used to receive and indicate the ~'clative amplitudes of fields, while that to the right IS used to produce VLF fields of appropriate fre­qyencr and amylitude. In calib~'ating , the deflec­tlOn of the recmver output m eter 111 response to the unlm~wn VLF field is obtained with the receiving loop .m the plane of propagation. The receiving loop IS then rotated 90 0 to minimize the receiver re­spo~l ~e to tbis field. The transmitting loop is posltlOned coaxially wi th the receivino' antenna at a separation distance of 1 or 2 m. Without chano-ina the recei:rer tUl:ing or sensitivity , the frequency band outpu t of the sIgna~ generator are adjusted to repro­duce the same receIver ou tpu t meter indication that was obtained in response to the unknown VLF field. The equivalent value of the radiation field inciden t at the . receiving antenna is calculated from eq (4) a,?ove 111 terms of the antenna radii, their separation dIstance, and the RF current in the transmitting an­tenna . T~le strengt~ o~ the unknown field is equal to the eqUlvalent radIatlOn component of the locally gener ated field.

In figure 2, the "Me tering Equipment" bloch:: is symbolic of the method used to determine t he RF current in the trans'~i tting loop . The technique is represented In detall m figure 3. Balanced RF voltages, obtained from t he RF signal generator and Balun (balanced-to-unbahlnced transformer) , are

FIGU RE 2. Block diagram of the loop antenna calibration system.

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SWITCHING ARRANGEMENT

THERMO­ELEMENT

LOOP ANTENNA

FIGURE 3. Calibration oj the transmitting loop antenna.

connected to the single-tum unshielded transmitting loop . A vacuum thermoelement is mounted in th e top-center of the transmitting loop as indicated. The RF current ll1troduced into the loop flows t hrough the thermocouple heater element. The d-c output voltage of the thermoelemellt is indicated by t he d-c Imlhvoltmeter. The RF current is then dis~onneeted from the loop antenna and replaced by a duect curren t . The direct curren t is adj usted to produce the same thermoelement d-e ou tpu t voltao'e that was attained in response to the RF cUlTe;t. Since equal values of I'ms RF current and direct current producc equ al thermoolement output volt­ages, the value of direct current read from the milli­ammeter, figure 3, is used in eq (4) in calculatino ' th e field strength at t he receiving loop antenna. b

. An RF micropotentiometer 2 [Selby, 1953] was ll:corporated mto the calibration cquipment to pro­VIde an accurate source of RF vol tages. '1'h e arrangement used f<?r calibrating the micropotenti­?meter and cstabhslnng known RF vol tages is shown 111 ~gure 4.. The thermoolemen~ of tbe micropo­tentlOmeter IS the same type used 111 the transmittino' l<?op . . Th"e switc.hing arrangement indicated permit~ eIther RB or dnect current to flow through the thermoelement and the micropotentiometer resistor element. To establish an accurately known RF volt~ge across the rnicropo tentiometer, the current req~lI'ed to produce the d esired voltage is calculated. A dll·e~t. curren t of ~ his magnitude (as indicated by t he mIlliammeter) IS caused to flow through the ther~110couple and resistor elem~nt of the micropo­tentlOmetel' . The d-c output of the thermoelement in response to the direct current is observed. An R! curr~nt of a-rpropriate frequency is then sub­s~l tuted for the (hrect curren t and adjusted in mag­l1ltude to produce the same thermoelement output voltage that was obtained in response to the direct current. The required RF voltage then exists across the resistive element of the micropotentiom­~ter. The mieropotentiometer, havin g an in ternal Impedance of a few milliohms, is usually used to ~alibrate equipm en t having inpu t impedances rang­mg from 50 ohms upwards. In such cases, the stand.ard voltage aeross the micropotentiometer is not slgmficantly altered when the equipment under calibration is connected.

, 'l' his is Simpl y a low·impedance sotU'ce of RF voltage adjustable from 1 to lO'J'v

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R F SOURCE

SWITCHING ARRANGEMENT

THERMO­ELEMENT

MICROPOT ENTIOM ETER

RESISTANCE ELEMENT

FIGU RE 4. Calibration oj the micropotentiometer.

4 . Description of Equipment

A ph<?togr~ph of t!le prototype of the field in tensity a~d cah?ratlOJ1 eqUIpm ent is given in figure 5. As vlCwed hom loft to right, the individual i tems are: The receiving loop an~enna shown connected by a cable to a box con tammg a balanced-to-unbalanced electrostatically shield ed tnlns f'ormer. The thjrd unit from the left is a transistori zed VLF receiver. The ne~t item is a commercially made transistorized VLF s~gnal generator. The transmitting loop an­te!lna lS ~hown mou~lted on a supporting pede tal wlth the mput termmals near the bottom and the ther~10~lement and its O~ltpu t ~t the top . The small box l~ iront and. to t!le nght 01 the tran smitting loop con tams a tran IstoI'lzed fmal amplifier for the signal ge~erator . T~le large ?<?x at the cxtreme right is the ca.h~ratlOn umt contau:lI:g the laboratory type d-c ~111hammete!' an~l d-c mIllIvolLmetcl', the micl'opo ten­tlOmet?r, sWltcbmg circuits, etc. A photograph 01 a collap Ible frame . to suppor t t ~ e. transmi tting loop a.ntenna (to the .left) and the l'CeClvmg antenna (to the rIgh t) IS shown 111 figUl'e 6. The spacinO' between the loop a~ltennas in this photograph is 2 m.b The frame­work IS made of shor t sections or tu bino' which may be disassembled in to a "bundle of sticl\:s" 1'01' easy transport.

FIGURE 5. Field intensity and calibralion equipment.

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FIGURE 6. Loop antennas mounted on a collapsible f rame f or fi eld use.

Although all of the equipment shown is battery­operated and has been used in field work, no serious effort was made to minimize the size or weight of this prototype equipment. Obvious improvements could be made, such as reducing the diameter of the receiving loop and the input transformer, positioning the final amplifier within the signal generator, minia­turizing the calibration unit, etc.

The receiving loop antenna is electrostatically shielded and balanced with respect to ground. The input transformer is a balanced-to-unbalanced unit with an electrostatic shield betweeen the primary and secondary windings. A high degree of balance was achieved in the loop input circuit to minimize undesirable unbalanced currents.

The transistorized, battery-operated VLF receiver shown in the photograph is an early model developed at NBS. An improved model has since been devel­oped which has a sensitivity of about 100 }Jov/m and a bandwidth adjustable from 40 to 400 cis. The receiver is tunable from 14.5 kc/s to 22 kc/s and is provided with a voltmeter to indicate the relative amplitude of received signals. In the experiment cited, voltmeter readings were made during intervals when station NLK was transmitting a steady carrier signal. It is intended to describe this receiver in a future publication.

.----------- - - - -- -- - - -- - - - - ---- - - -- -- - - -- ---- --------..., I I

, , , , , , i , , +

5-IO-20mv

SHUNT ;

· 5-10-20 : I

i I I ,

\..1 "~';;"' -' \\, 0--------+-1----1 .....

RF GEN

, I I I I

I I l ~ RG-22 I , L __ _________ ___ ___________ ___ _______ -- - -oJ

FIGU RE 7. Schematic of calibration unit.

RG-22

A schematic diagram of the calibration unit is shown in figure 7. The apparatus for the generation of standard fields (represented in fig. 3) and for the calibration of the micropotentiometer (represented in fig. 4) are combined in this unit. The d-c milliam­meter and millivoltmeter are high quality laboratory instruments with accuracies of 0.5 percent. Thermo­elements of 5- to 100-ma capacity were used in the micropotentiometers, which enabled standard volt­ages to be generated within a range of 100 to 50,000 }JoV with an accuracy of better than 3 percent. This type of thermo element when calibrated with direct current can be used as a current-measuring device up to 300 Mc/s to an accuracy within 1 percent.

The transmitting loop consists of a single-turn unshielded loop with a 100 rna thermoelement mounted in the top-center. The balun transformer has a voltage unblance that is less than 2 percent of the balanced output voltage, and an insertion loss that is less than 0.3 db. This i:lystem can be used to establish standard fields with excellent precision and an accuracy that is better than 5 percent.

The transmitting and receiving loop antennas, with radii of approximately 0.1 and 0.35 m, respective­ly, were spaced 2.0 m from each other. Under these conditions the bl'acketed series in eq (4) yields a correction factor of approximately 1.028. This repre­sents an increase of approximately 3 percent over the value of the field if the correction is neglected.

The equipment described in this paper was de­signed to measure field strengths in the range from 230 to 23,000 /lv/m at frequencies between 15 and 20 kc/s. The range of frequency coverage can be extended by proper selection of the balun trans­former, the signal generator, and the receiver. The micropotentiometer can be used over a voltage range of 1 }JoV to 200 mv at frequencies up to 300 Mc/s.

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-------- ---- --

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The ranges of operation of this equipment can be exLended in frequency and amplitude [or use in other applications. Excellent precision is obtained with this system with an accuracy not before attainable. All calibrations are performed with direct current. This eliminates many sources of error, and the d-c measuring instruments can readily be checked against reliable d-c working standards. This unit was recalibrated after an extensive field trip , and the calibration of the instruments did not vary more than 0.2 percent.

5. References

Dwight, H . B., Tables of integrals and other mathematical data, Revised edition (MacMillan Co. , New York, N.Y., 1947) .

Greene, F. M ., Calibration of commercial field strength metcrs at the National Bureau of Standards, NBS Circ. 517 (D ec. 1951).

IRE Standards on radio-wave propagation, Measuring Methods (1942).

Selby, M. C., R. F. Micropotentiometers, Radio-Electronic Engineering (Oct. 1953) .

Smythe, W. R., Static and dynamic electricity (Mc Graw-Hill Book Co., Inc., New York, N .Y., 1950).

(Paper 6503- 70 )

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