ionospheric sounding using coded pulse signals

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RADI O SCIENCE Journal of Research NBS / USNC-URSI Vol. 68D, No. 10, October 1964 Ionospheric Sounding Using Coded Pulse Signals 1 D. C. CoIl and 1. R. Storey Contri bution From De pa rtme nt of Nation al Defence, Defence Re sea r ch Board, Defence Re sea rc h Telec om- muni ca tions Establi shment, Shirley Bay, Ottawa 4, Ontario, Can . (Recei ve d Apri l 8, 1964) At present , iono sp heric so und ers rely on t he transmission of high peak-pulse -power to provide for t he detection of received ec hoes. To allow for the detect ion of signals with pOOl' signal- to-noise ra t io s, t he transmitted ene rgy mu st be incr eased . It can be ass umed that significant increases are no t likely to be obtained through increases in the pea k tr ans - mi tte d power. Also, an y increase in trans mitted ener gy ac hi eved thro ugh a simple increase in pulse duration is acco mp anied by a corrcsponding loss of ra nge resolu tion. Pul se com- prcssion si gna ls provide an i ncrease in transmi tte r! energy, wi t hout an inc rease of pea k power, a nd "' ithout a loss of range resolution . Thi s paper describes an a ppl i cat ion of pulse-coded pul se co mpr essi on s ig na ls to the field of ionospheric so unding. Th e signals used an d the ir properties, their generat io n an d reception, and the perfo rman ce of an experimental vertical so und er ar e discusse d. Th e e ff ects of ionospheric a nd syste m perturbation s on performance are also cons id ere d. 1. Introduction The use of pulse sounding techniques for iono- spheric inves tigation is now widespr ead. So undin g is employed for sci en tilic purposes, fr equency pre- diction purposes, and for real-time assistance to HF communic at ion systems. Pulse transmi tters are used in con junction with suit able receiv ers to ver- tically so und bo tb the bo tto m and top of t he ion o- s phere, and to obliquely so und long-di sta n ce ionospheri c p at hs b et wee n points on the ec),rth's surface. By employing precise Liming uni ts for t he gener at ion of the pulse repetition J' flte, as well as for frequen cy co n t rol , the tra nsmit ter and receiver are maintained in synchr o ni sm ,),s they are swept across a p ort ion of the high. frequency sp ectr um (3 to 30 Mc/s). The Defence Research Tel eco mmuni cation s Estab- lishment (DRTE) bas had an int erest in ionospheric sounding for man y years [Cox and Davies, 1955 ; Cha pman, D avies, and Littlewood, 1955 ; Hatton , 1961 ; Jull , Doyl e, Irvin e, and Murray, 1962], and bas been concerned with the implementa tion of signal processing techniques for improving the per- forman ce of so under s [ColI and P oaps, 1964]. Sounders normally rely upon the trans mi ssion of a pulse of RF en er gy with a shor t dur at ion, to provide the desired reso lution b et ween ionospheri c propaga- tion modes ; and with a high pe<tk power, to provide the desired system sensitivity. Because of the use of n arrow pulses, so undin g receiver band widths of 30 to 100 kc /s are co mmon ; therefore, so undin g re- ceivers tend to be more susceptible to interference than normal HF communic at ions equipment . 1 Paper prescn ted at tho 1963 Fall URSI Meetin g, Seattle, Wash. , Dec. 9-11, 1963. For r eception of so undin g signals in hi gh inter- ference environments, or wh en the signals are low, it is necessary to incr ease the energy in the trans- mitted signal. In the past, in creased transmitted ener gy has been ac hi eved by in creases in the peak of th e mittel', unti l, now, peak powers of t h. e order of 100 to 200 levV are not un - co mmon. It does not app ear that significant in- creases in transmi tted ener gy can be obtained througll increased p eak powers since severe difficul- ties a ri se in the des ign of tran s mi tter s, tunable over the HF band , if t he peak power is over 100 kW. Also tran smi tters with such powers can cause local interf er ence. is possible to increase the trans mitt ed en ergy by mcreaS ll1g the pulse len gt h. Tl li s has two a d- verse effects: first, the range resolution of the shor ter pulse has been lost; seco nd , ener o'y of the lon o'er pulse is co ntain ed in a narr ower bandwidth :nd thus will cause more interference to communication systems opera ting on the same frequ encies. A solution th at has been implemented at DRTE t .'l e of. co ded pul s.e signals, i. e., signals con- of tral11S of co nti guous, rectangular, pulses ll1 which each component pulse is s uit ably co ded. Such signals can hav e an ener gy comparabl e to that of a long pulse, a nd have resolu tion simil ar to that of a single pul se with a dur ation equal to that of one of the componen t pul ses of the train . 2. Coded Pulse Signals si gnals used in the s ounding system co nsist of of component pulses. A matched filter is used 111 recei,ver to maximize the ignal-t o- white-noIse ratlO. 'lhe res ponse of this matched fil ter, wi th the signal as an input, will d etermine the. 11 55

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RADIO SCIENCE Journal of Research NBS/USNC-URSI Vol. 68D, No. 10, October 1964

Ionospheric Sounding Using Coded Pulse Signals 1

D. C. CoIl and 1. R. Storey

Contribution From Department of Nation al Defence, Defence Research Board, Defence Resea rch Telecom­munications Establishment, Shirley Bay, Ottawa 4 , Ontario, Can.

(R eceived April 8, 1964)

At present, ionospheri c so unders rely on t he transmission of high peak-pulse-power to provide for t he detection of rece ived echoes . To allow for t he detection of signals wit h pOOl' signal-to-noise ra t ios, t he transmitted energy must be in creased . It can be ass umed that significa nt increases a re not likely to be obtained t hrough increases in t he peak t rans­mi tted power. Also, an y increase in t ra nsmitted energy ac hieved t hrough a simple in crease in pulse duration is acco mpa nied by a corrcsponding loss of range resolu t ion . Pulse com­prcssion signals provide an increase in t ransmi tte r! ene rgy, wi t hout an increase of peak power, a nd "' it hout a loss of range resolution .

This pape r descr ibes an a ppl ication of p ulse-coded pulse co mpression sig na ls to the field of ionospheric so unding. The signals used an d t heir proper t ies, t he ir generation an d rece pt ion , a nd t he perfo rm a nce of a n exper ime ntal vertical so under are discussed. The e ffects of ionospheric and syste m perturbations on performance are also cons ide red.

1. Introduction

The use of pulse soundin g techniqu es for iono­spheric investigation is now widespread . So unding is employed for scien tilic purposes, frequency pre­diction purposes, and for real-time assistance to HF communication systems. Pulse transmitters are used in conjunction with suitable receivers to ver­tically sound bo tb the bottom and top of t he iono­sphere, and to obliquely sound long-distance ionospheric paths between points on the ec),r t h's surface. By employing precise Liming uni ts for t he generation of the pulse repetition J' flte, as well as for frequency con t rol , the transmitter and receiver are maintained in synchronism ,),s they are swept across a portion of the high. frequency spectrum (3 to 30 Mc/s).

The Defence R esearch Telecommunications Estab­lishment (DRTE) bas had an interest in ionospheric sounding for many years [Cox and Davies, 1955 ; Chapman, D avies, and Littlewood, 1955 ; Hatton, 1961 ; Jull, Doyle, Irvine, and Murray, 1962], and bas been concerned with the implementation of signal processing techniques for improving the per­formance of sounders [ColI and P oaps, 1964].

Sounders normally rely upon the tr ansmission of a pulse of RF energy with a shor t duration, to provide the desired resolution between ionospheric propaga­t ion modes ; and with a high pe<tk power, to provide t he desired system sensitivity. Because of the use of narrow pulses, sounding receiver band widths of 30 to 100 kc/s are common ; therefore, sounding re­ceivers tend to be more susceptible to interference than normal HF communications equipment.

1 Paper prescn ted at tho 1963 Fall URSI M eeting, Seattle, Wash. , Dec. 9-11, 1963.

For reception of sounding signals in high inter­ference environments , or wh en the signals are low, it is necessary to incr ease the en ergy in the trans­mitted signal. In the past, increased transmitted energy has been achi eved by increases in the peak pulse-po~e)' of th e t~'an mittel', until, now, peak powers of t h.e order of 100 to 200 levV are not un­common. It does not appear that significan t in­creases in transmi tted energy can be obtained t hrougll increased peak powers since severe difficul­ties arise in the design of transmi tters, tunable over the HF band, if t he peak power is over 100 kW. Also transmi tters with such powers can cause undesirabl~ local interfer ence.

I~ is possible to increase the transmitted energy by mcreaSll1g the pulse length. T llis has two ad­verse effects: first, the range resolution of the shorter pulse has been lost; second, ~he enero'y of the lon o'er pulse is contained in a narrower bandwidth :nd thus will cause more interference to communication sys tems opera ting on the same frequencies.

A solution t hat has been implemented at DRTE i~ t.'le us~ of. coded puls.e signals, i. e., signals con­~nstll1g. of tral11S of contiguous, rectangular, pulses ll1 which each component pulse is suitably coded. Such signals can have an energy comparable to that of a long pulse, and have resolution similar to that of a single pulse wi th a duration equal to that of one of the componen t pulses of the train .

2 . Coded Pulse Signals

~he signals used in the sounding system consist of ~rall1s of component pulses. A matched filter is used 111 ~he s~undin~ recei,ver to maximize the ignal-to­white-noIse ratlO. 'lhe response of this matched fil ter, wi th the signal as an input, will determine the.

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advantfLge of the pulse compression signals over a single pulse signal. The output of the matched filter due to signal alone, is the autocorrelat,ion function of the signal; and the output signal-to-noise ratio depends only on the energy in the signal and the power spectral density of the noise [Turin, 1960). It is necessary, then, to design signals whose auto­correlation functions approximate that of a single pulse. Unlike the general radar case, there does not appear to be a requirement on sounding signals for Doppler resolution.

A signal that consists of a train of N pulses may be represented by a sequence of elements, a i, where the a i are the signals in each pulse. The autocorrelation function , p(k) , of the signal is given by the expression

and

r N- I -k

(k) _ { ~ aiai+k p - 1=0

o

O-::;'k-::;'N-l

k> N-l

p( -k) = p(k) .

If the response of the system may be considered , for all practical purposes, to exist for only one com­ponent pulse duration (i .e., only for k = O), then the signal will have the same range resolution as a single pulse with a duration equal to that of a component pulse. In terms of the expression above, it is desir­able that the autocorrelation function be made small for all nonzero values of k. The values of p(k) for krfO are called the side lobes of p(k), because of the similarity between the desired form of the autocor­relation function and a narrow-beam antenna pattern. The value of p(O) is equal to the energy in the signal, and should be maximized relative to the side lobes. If the side lobes are low, the possibility of confusing a low-level multipath echo with a side lobe caused by a stronger echo is minimized. That is, ambiguities between side lobes in the response and multipath echoes are minimized. Two parameters that are used to com­pare signals are the peak-to-maximum side-lobe ratio , and the energy of the signal relative to that of a single component pulse with the same peak power.

The design of pulse signals, in which either the amplitude or the phase of the individual pulses has been coded, has received considerable attention in the literature [Turin, 1960; Huffman, 1962; and Frank, 1963). In particular those signals in which the a i are constrained to be either + 1 or - 1 have been thoroughly investigated. Such binary codes are particularly simple to generate. Signals in which the ai are allowed to be any complex number have been discussed by Huffman (1962). He has specified necessary and sufficient conditions such that p(k) = O for krfO or (N-l). Huffman has called these signals "impulse-equivalent pulse trains ." For convenience, they are referred to in this paper as "Huffman" signals. It is also possible to restrict the a i to be elements from a finite set of unit vectors, each with a distinct phase [Frank, 1963). Such signals are called polyphase codes.

3. Experimental System

The specific signals used in the experimental sounding system were:

(a) Single pulses, (b) binary codes of length 17, and (c) impulse-equivalent pulse trains of length 17.

The basic pulse length used was 25 }.I.sec, and the signals were transmitted as double-side-band sup­pressed-carrier at a peak power of 1 kW.

The single pulse and binary waveforms are shown in figure 1. The single pulse, of amplitude + 1 and duration T seconds, and one-half of its (symmetrical) autocorrelation function are shown on the bottom right-hand side of the figure. The binary pulse train, of amplitude + 1 or -1 and overall duration 17 T , along with its autocorrelation function, are shown to scale. The peak value of the correlation function (equal to the energy of the signal and the peak output of the matched filter) is 17, compared to 1 for the single pulse. The side lobes, values of the correlation function for nonzero shifts, can be seen. The peak-to-maximum side-lobe ratio is 17 to 2 or 8.5:l.

The impulse equivalent pulse train is shown in figure 2, with one-half of its autocorrelation function. This signal has only one component pulse with a magnitude of 1 and hence has less energy than the constant magnitude binary signal. The energy in the Huffman signal is 7.28 times that of a single pulse of the same peak amplitude. The peak-to­maximum side-lobe ratio 2 is 10.8. The simple form of the autocorrelation function is very evident in figure 2. Note that multipath echoes would be detectable without ambiguity, as long as they did not fall upon the single side lobe.

2 The Huffman signa l of len gth 17 with m aximum energy (and peak amplitude I ) has an energy 01 8.26 times that of a single pulse and a peak· to·side lobe rati!> of 8.26.

17

16

15

14

13

12

II

10

6

4

-, -2

\BINARY PULSE TRAIN

+'1 firinnn -~ LJ 0 u uv

AUTOCORRELATION FUNCTION OF BINARY PULSE TRAIN .

~CPULSE T

AUTO CORRELATION FUNCTION

OF SINGLE PULSE. ~

"""'>--f"'!;T---

FIGU RE 1. S ingle pu lse and binal'Y signals.

lIS6

One reason for the interest in pulse train signals is the simplicity with which they may be generated and received. The signals ar e generated in a tapped shift-regis ter delay line, as shown in figure 3. A single logical 1 is shifted down a 16 element shift register at a 40 kc/s shift rate. This places a voltage successively on each of 17 taps. These voltages are summed with t he appropriate weighting to form th e signal. The signal is then used to modulate a carrier in a balanced m odulator which feeds a wideband linear power amplifier . The carrier frequency can be tuned from 2 to 24 M c/s.

Because of t he bipolar nature of the signal a phase sensitive receiver must be used . Filters, matched to the low-pass signal, are used in a quad­r ature detector as shown in figure 4. In this receiver , the IF signal, J(t)cos(wl+ lJ) is multiplied by signals from a local oscillator in two separate phase-sensitive detectors. These local oscillator signals are in phase quadrature. [In the figure it is assumed that there is a frequency difference ilw , a nd a phase shift IJ, between the received signal (at the IF ou tpu t) fmd the local oscillator :] The low-pass output of til e ph ase-sensitive-detector in each arm is applied to identical fil ters, matched to the signal J(t). The filter outputs are squared and added. If the fre­quency difference is negligible, the receiver output will be the squared correlation function .

The matcbed fil ter is sbown in figure 5. It co n­sists of a finite-t ime-integra tor (matched to a single, 25 j.Lsec, rectangular pulse) followed by a linear , tapped, delay line. The gain of each tap is adjusted so that the impulse response of t he matched fil ter is the time inverse of th e signal.

The waveforms generated in the experimental system are shown in figure 6 along wi t h the cor ­responding matched fil ter outputs. In the case of the Huffman sig nal , it can be seen from the photo­graph that any side lobes caused by depart,m es of the system from the ideal, are less th an t he legitimate side lobes.

e 7

6

4

IMPULSE EOUIVALENT +1 1 _____ PULSE TRAIN

.~J~-7.28

AUTOCORRELATION FUNCTION

O~---+·~----------__ · -I 0.674

17T -2

FIG UR E 2. I m plllse eqlLivalent pulse tmin.

SHIFT PULSES

40 kc/S PRF~

SINGLE

PUL 251Lsec sE-'

TAP GAINS ~ 9C

• • • • • 9 C ~C ~C 9 c 9 c ~ c ~C 9 C ge ~ e ~ C ~ C ~ c ge

L

i CARRIER BALANCED TRAN SMITTER

INPUT MOOULATOR DRIVE

SIGNAL GENERATOR

FI GU R E 3. Signal generatm·.

f(t)sinL~wt-8 )

a (t)= f OOf(Tlf (t- T ) si n ( A""T -8) dT .<D

FI G UR)" 4. ReceiveT.

FILT ER MATCHED TO 25fLsec RECTAN GULAR PULS ES r-- ----- ------------ , I I I

INTEGRATOR

9 c~

+

400fLsec ANALOG DELAY LINE TAPPED AT 25fLsec INTERVALS

OUTPUT

MATCHED FILTER

F I GUR E 5. lVlatehed filter.

SHIFT REGISTER

______ ~n~. -------- r-rrrr I ·~L~~L-.r-

:o-_~I A\o.. __ _ -.-__ J~ SINGLE PULSE BINAR Y

------"I.J l .... __ _

.~dJ1; .. HUFFMAN COMPARISON

F IGU R E 6. GeneTated wavefo1'lns and matched fi lter outputs.

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4 . Ionospheric Effects on the Signals

The discussion of signal design, generation, and reception in the previous section has neglected the fact that the signals are to be used for ionospheric so unding. Three effects, due to propagation and ionospheric reflection, are liable to affect the pulse compression capability of the system. They are

(i) Changes in the length of the propagation path during transmission of the signal. Such changes alter the relative phases of the received signal and the receiver local oscillator. That is , in figure 4, () becomes a function of time. This nonstationarity of the medit'm limits the length of signal that may be used.

(ii) Multipath . The superposition of multiple re­flections will distort the expected receiver output, due to the squarers in the quadrature detector. This effect limits the unambiguous determination of the relative amplitudes of multipath components.

(iii) Change of the propagation time with fre­quency. This effect limits the signal bandwidth that may be used . From a consideration of these points. it is clear Ghat pulse compression will be most effective during times of stable conditions, at frequencies removed from the critical layer frequencies , and will be most useful for the qualitative detection of echoes that would otherwise be obscured by noise. It will work during disturbed conditions, but with reduced efficiency.

5 . Performance

The signals described above were tested on a vertical sounder at Ottawa, Ontario during Septenl­bel' 1963. The sounder was tunable, but was oper­ated at suitable fL'{ed frequencies. The dramatic advantage of the pulse compression signals, i.e ., the improvement in signal-to-noise ratio relative to that of a single pulse, is shown in figures 7 and 8. To make these oscillographs, the system gains were adjusted to equalize the output noise levels. Figure 7 shows A-scan photographs of two transmissions, separated in t ime by 100 msec. The time bases used were approximately 3 msec long in each case. The echoes that are just barely discernible in the single pulse case are clearly evident in the bin arT case. Similarly, in figure 8, a Huffman signal and a single pulse are compared, the two photographs being taken 100 msec apart. It is in situations such as these that pulse compression signals will be most useful.

The advantage of impulse-equivalent pulse trains over binary ones, from the point of view of side lobe ambiguity, is demonstrated in figure 9. H ere, the response to a Huffman signal is shown on the left and the response to a binary signal transmitted 100 msec later, on the right. The tiTne scale is 200 /lsec per division. The absence of side lobes on the Huffman signal is evident in the interval between the extraordinary echo (in the middle of the each trace) and the dispersed, high-amplitude ordinary echo (at the right-hand-side of each trace). In the

PULSE

... . . Jh I 1.' ....-.a BINARY

FIGU R E 7. Improvement in signal-lo-noise Talio.

PULSE HUFFMAN

FIGURE 8. Imp1'ovement in signal-lo-noise Tatio.

HUFFMAN BINARY

FIG liRl,} 9. Comparison of HlI:ffman and binary signals.

binary case, it is difficult to distin guish b etween the extraordinary echo and the side lobes of the ordinary echo.

6. Conclusions

Experience gathered with the experimental equip­ment indicates that a varietT of signals should be available 1'01' sounding purposes. The signal used at any time would depell(l on the specific req uire­ment, propagation conditio ns, and interference en­vironment. To achieve best performance uncleI' all conditions, so unders )\lust be ahle to adapt to n1.eet each new set of conditions.

Single pulses are ideal:v the best signals for sound­ing. For those situation s in which high signal-to­noise ratios exist single pulses should be used .

Huffman signals may be used to achieve increased detectabil ity with a minimum of side lobe ambiguity. They may also prove useful in providing sounding systems using lower peak powers than the HF sound­ers now in operation. This would be of particular advantage for mobile sounding installations in satel­lites or aircraft.

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Binary signals should be used to provide maximum detectability when signal-to-noise rfltios are poor. They also are the simplest to instrum ent , and might find application in digital systems.

In comparing the performance of various signals it is worth noting thflt if the provision of added energy in the signal, in the form of pulse co mpression codes with reasonable peH,k-to-side-lobe ratios, allows the detection of echoes previously obscured by noise, then the problem of sidelobe ambiguity is of second­ary importance.

7. Future Experiments

The equipmen t used in this study is being prepared for oblique sounding applications. It will be oper­ated in conjunction with programmable frequency synthesizers to provide stepped frequency sounding from 2 to 24 M c/s over a 1000 km path .

(Paper 68DIO- 415)

8. References

Chapln:tn , J . 1-1. , K . D avies, and C. A. Li ttlewood (1955), R ad io obse rvat ions of the ionosphere at oblique in cidence, Can. J . Phys. 33, 713- 722.

Coil, D. C., a nd G. E . Poaps (Jan. 1964), A video s ignal enha nce r fo r improv ing t he pe rfo rma nce of oblique incidence ionosphe ri c sounde rs, DRTE Techni cal Report No. 1127.

Cox, J. W ., a nd Ie Davies (1955), Ob lique incidence pulse transm iss ions, Wireless E nginee r 32, 35- 41 .

Frank, R. L. (Jan. 1963), Polyphase codes with good nOIl­periodic correlation proper ties, I EEE Tra ns . Inform . Theory IT- 9, No. 1, 43- 45.

Ha tton , W. L. (Sept. 1961), Oblique-sounding a nd HF radio communication , IRE Trans. Commun . Syste ms CS- 9, No.3, 275- 279.

Huffman , D. A. (Sept. 1962), The generation of impulse­equivalen t pulse "trains", IRE Trans. Inform . Theo ry IT- 8, No.5, s10- s 16.

Jull, G. W., D . J . Doyle, G. W . Irvine, and J. P. Murray (July 1962), Frequency sounding techniques for HIi' com­munications over a uroral zone paths, Proc. IRE 50, No . 7, 1676- 1682.

Turin , G. L. (June 1960), An in t rodu ction to matched filte rs, IRE Trans . Inform . Theory IT- G, No.3, 311- 329.

Wa rre n, E. S. (Nov. 1962) , Sweep-frequency rad io soundings o f t he top s ide of t he ionosphe re, Can . J . Phys. <10, p. 1692

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