System for Analyzing Time-Dependent Phenomena

This invention relates to systems for time-resolving data, and particularly to the time resolution of data multiplex-encoded into a single channel.

For example, conventional analysis of spectral phenomena typically involves a plurality of observations of each spectral element over a period of time. Such observation can be made in parallel along a like plurality of channels or can be made sequentially over a single channel. Effectuation of such a series of sequential observations is highly inefficient because the total time during which any one resolution element (e.g. a particular wavelength band) can be observed practically is quite limited. Additionally, the observation of each resolution element implies that all of the other data are discarded or unused during the particular observation time. A resolution element here can be defined as the number of samples to be taken of a phenomenon, divided by the total time required to obtain the totality of samples.

Fourier transform spectroscopy provides a substantial improvement over the classical dispersive techniques exemplified by a conventional spectrometric single channel method. A Fourier transform spectrometer provides a sequence of data generated on a single channel and arising from the modulation of all wavelengths of input light with a separate carrier frequency. The separate wavelengths can then be discriminated from one another by frequency filtering, the amplitude of each frequency being proportioned to the intensity of the light at the wavelength corresponding to that frequency. Such an interferometer spectrometer can thus measure wavelength for a time N/2 (where N is the number of resolution elements) longer than the time required to obtain similarly resolved measurements with conventional spectroscopes. The improvement in accuracy gained by using an interferometer spectrometer (i.e. the square root of N/2) is known as Felgett's advantage or the multiplex advantage, and is described in detail by L. Mertz, Transformations in Optics, Chap. I, John Wiley & Sons, Inc., (1965). Such Fourier transform spectroscopes usually either employ stepping interferometers with gated detector signals or incorporate rapid scan techniques. The former imposes severe limits on instrument stability as well as source life time; the latter imposes severe limits on maximum achievable resolution, signal-to-noise ratio and time resolution.

Spectroscopy with a rapid scan interferometer has been considered most useful with steady-state or quasi steady-state light sources because, as Mertz points out, where there is source modulation, the noise level increases by N/2, as compared with Felgett's advantage of square root of N/2, leaving a net inferiority of a factor of the square root of N/2. In effect, the modulation of the source is considered to act as a factor similar to a truncating function. For the foregoing reasons, the use of Fourier transform spectroscopy to examine time-varying spectral phenomena has been largely neglected despite the extremely efficient throughput of a Fourier transform spectroscope.

R. E. Murphy et al in "Time-Resolved Fourier spectroscopy" Journal of the Optical Soc. of America, Vol. 65, No. 5, May, 1975, pp. 600-605 suggests that Fourier spectroscopy can be used to investigate time-dependent spectral sources. Murphy et al observed with an interferometer-spectrometer a series of phenomena each at a different fixed path retardation, synthesized from the data a set of time sequenced interferograms and transformed the time-sequenced interferograms to obtain the recovered spectra at successive time intervals. However, the Murphy et al technique, using stepped retardation, is subject to the limitations on instrument stability and source life time above noted and is highly sensitive to amplitude variation among the several phenomena observed.

The present invention overcomes problems of the prior art by employing both temporal and spectral multiplexing with a transform system which allows high resolution and signal-to-noise even with data with microseconds resolution time. A principal object of the present invention is therefore to provide means for a method of analyzing transient phenomena using both temporal and spectral multiplexing. While the system can be used with any of a large number of data gathering devices (such as pulsed NMR and NQR systems, Hademard spectrometers and the like) particularly, the present invention has an important object the use of a continuous scanning Michelson interferometer for spectral study of kinetic systems using both temporal and spectral multiplex techniques.

To effect the foregoing and other objects, the present invention generally is embodied in a system for time resolving a sequence of data derived from a phenomenon, which system comprises repetitive initiation of the phenomenon, detection of each occurrence or cycle of the phenomenon and the repetitive convolution with a transformation (as by continuous, controlled-velocity, repetitive, interferometric scanning) to provide an ordered set of interferograms each being representative of the course of each cycle of the phenomenon. By establishing the repetitive scanning cycle and the repetition of phenomenon initiation at different repetition rates, the scanning, and excitation cycles therefore are shifted in time in ordered increments with respect to one another preferably until the intitial temporal relation between initiation and sampling is restored. The term "interferogram" as herein used refers particularly to a self-reciprocal transform of a time sequence of input data, e.g. a Fresnel, Fourier, Dirac or other such transformation where the input data are spectral, sonic or the like. From the first set of interferograms, at least one "time average" interferogram is synthesized from a plurality of data moieties or points, each being at the same selected fixed position (in time) on each of the first set of interferograms with regard to initiation of the phenomenom. The "time averaged" interferogram (or second set of interferograms as the case may be) is then analyzed or subjected to the inverse of the initial transform to produce a data set representing the phenomenon as it occurred at that fixed data point in time following initiation of the phenomenon, i.e. the data set is constant in "source" time. Alternatively, each interferometer scan is sampled only once at a present time following initiation of the phenomenon, all samples taken during scans having the same retardation phase relative to initiation being coadded to provide an average signal. The time relation between a selected retardation point in the interferometer and phenomenon initiation is periodically shifted to produce a series of such average signals. The latter can be assembled in time sequence to synthesize the "time averaged" interferogram.

Other objects of the invention will in part be obvious and will in part appear hereinafter. The invention accordingly comprises the apparatus and method possessing the construction, combination of elements, and arrangement of parts which are exemplified in the following detailed disclosure, and the scope of the application of which will be indicated in the claims. For a fuller understanding of the nature and objects of the present invention, reference should be had to the following deetailed description taken in connection with the accompanying drawings wherein:

FIG. 1 is a schematic block diagram of a system embodying the principles of the present invention;

FIG. 2 is a number of representative idealized waveforms on a common time base, of signals appearing at various points in a system of the type shown in FIG. 1;

FIG. 3 shows representative spectra obtained by transformation of interferograms synthesized from other interferograms taken during photolytic decomposition of acetone;

FIG. 4 shows representative spectra obtained by transformation of some synthetic interferograms derived from the photolysis of acetaldehyde;

FIG. 5 is a schematic block diagram of an alternative version to the system of FIG. 1; and

FIG. 6 is a number of idealized waveforms on a common time base of signals appearing at various points in a system such as that shown in FIG. 5.

The present invention can advantageously be described typically in connection with scanning interferometric means as an examplary means for generating interferograms each being representative of at least some stage in the progression of a phenomenon being observed. The latter, for examplary purposes here, will be considered to be the photolytic decomposition of acetone vapor by ultraviolet radiation, although it should be appreciated that a very large number of phenomena are susceptible of analysis by the present system. For example, the invention can be employed in basic chemical kinetics studies, isotopic separation processes, laser fusion phenomena, phototchemical ionization and free radical phenomena, relaxation phenomena and the like. The present invention is particularly useful in study and analysis of processes in which excitation occurs within 10.sup.-6 to 10.sup.-8 seconds, and after approximately 10.sup.-4 seconds the excited medium relaxes eithin about a 10.sup.-3 to 10.sup.-1 second period.

As typical scanning interferometric means, one can use a Digilab Model FTS-20, commercially available from Block Engineering, Inc., Cambridge, Massachusetts. As shown in FIG. 1 such an interferometric means typically includes white light source 20 and monochromatic light source 22, both positioned to illuminate the entrace aperture of reference interferometer 24. The latter typically is a Mechelson interferometer in which the scanning element serving to modulate input radiation to provide an interferogram thereof, is a movable mirror shown schematically at 26.

Positioned in known manner to detect the modulated interference pattern produced by reference interferometer 24 are broad band white light detector 28 and monochromatic light detector 30, it being understood that these detectors include any filters necessary to discriminate between the interference patterns respectively produced in response to the respective light sources.White light detector 28 typically produces an electrical signal as a function of the white light interference pattern or interferogram generated by reference interferometer 24. The electrical output of detector 28 is coupled to the input of amplifier 31 and the output of the latter is connected to the input of a threshold-and-peak detector circuit 32.

Similarly, detector 30 provides an electrical signal as a function of the light input thereto, to the electrical output of detector 30 is coupled to the input of amplifier 33. The output of amplifier 33 is connected as an input of zero-crossing square wave generator 34. The latter typically is simply an axis-crossing detector circuit, the output of which is coupled to the input of a monostable multivibrator or one-shot to trigger the later to produce a square wave when an axis-crossing is detected. Both circuits being well known in the art so need no further delineation. The output of axis-crossing detector 34 is connected to the input of integrating servo loop circuit 36. The output of servo loop circuit 36 is connected to the input of linear ramp signal generator 38. The output of the latter is connected through power amplifier 40 as the input to drive motor 42, typically a solenoid-type reciprocating motor.

The interferometric means also includes sampling interferometer 44, substantially the same as reference interferometer 24, in which the scanning element which serves to modulate input radiation is shown schematically and typically as mirror 46. Both mirror 46 and mirror 26 are connected by a mechanical coupling (shown schematically at 48) to motor 42 so as to be driven synchronously by the latter.

Disposed with respect to interferometer 44 so as to detect the interference pattern of interferogram produced by the latter, is detector 50 which serves to convert the optical interferogram into a corresponding electrical signal. The electrical output of detector 50 is coupled through amplifier 52 to the input of analog-to-digital converter 54, and the output of the latter is connected through appropriate interfacing (not shown) to computer 56. The interferometric means thus described is essentially the prior art basic structure of the aforesaid commercial FTS-20 device. Computer 56 is typically a Nova Model 2/10 computer (commercially available from Data General Corporation, Southboro, Massachusetts coupled to a 1.2 million word moving head disc for temporary data storage and a digital magnetic tape for permanent data storage and constitutes a convenient form of means for selecting from each interferogram of an ordered set, a data point corresponding to a time resolution element of interval occurring at a fixed time position following initiation of the phenomenon, and for combining the data points in the same order as the ordered set to synthesize a second interferogram representing the convolved data only at that time position. It will be apparent to those skilled in the art that a dedicated special purpose digital computer or hard-wired analog system could readily be substituted in place of computer 56.

The means for repetitively initiating the phemonemon to be analyzed includes sample chamber 60 in which the phemonemon is to be initiated, and triggerable excitation source means 62 for exciting the phemonenon of interest in chamber 60 at selected times. Typically, chamber 60 is an enclosure such as a 30 centimeter long quartz absorption cell equipped with KBr windows to permit detection of the phenomenon by infrared absorption. To this end, infrared souce 64 is disposed for illuminating sample chamber 60 such that interferometer 44 can modulate infrared radiation emitted from chamber 60 following any infrared absorption occurring in the course of the phenomenon. Excitation source means 62 can be any of a number of systems, but typically, for the example of photolytic decomposition chosen here, is a triggerable ultraviolet flash lamp system as a 1540 Strobolume system (commercially available from General Radio Company, Concord, Massachusetts) which can provide a 1/4 joule output intensity 10 .mu. sec. full width, half-maximum light pulse.

Source 62 is also connected to be controlled by trigger circuit 66. Thus the source can be triggered at any selected time at any of a number of selected rates. The output of generator 34 is connected to the input of pulse generator 67, typically a Schmitt trigger circuit, the output of the latter being connected together with the output of detector circuit 32 as inputs to AND gate 68. The output of the latter is connected to the inputs of both delay circuit 70 and divider 72. Delay circuit 70 which simply serves to introduce, in known manner, a time delay into signal propagation, has its output connected to the reset input terminal of sample-and-hold circuit 74.

The system of the present invention provides means for converting into digital form each sequence of data produced by interferometer 44. To this end, the data input terminal of circuit 74 is connected to the input of analog-to-digital converter 54, so that circuit 74 serves as a sampling linkage between interferometer 44 and computer 56.

Divider 72, a typical digital "divide-by-N" circuit, has its output connected to the count input of a settable delay means such as counter 76. The count in the latter is typically controlled or selected by manually operable setting switches 78 such as thumb wheel switches or the like. Lastly, the output of detector circuit 32 is also connected as an input to the reset terminal of counter 76.

In operation, drive motor 42 is driven by a linear ramp or sawtooth signal from generator 38 so that mirrors 26 and 46 have a displacement velocity of approximately 0.3cm/sec. The light from source 22 (typically an HeNe laser which provides an output at 6328 A) is modulated by the motion of mirror 26, and because the mirror motion is linear, detector 30 and amplifier 33 provide a sinusoidal output (shown schematically at FIG. 2A) witha period of approximately 100 microseconds. Similarly, white light detector 28 will provide a well known white light interferogram as the path retardation of interferometer 24 changes with the motion of mirror 26. Such a white light interferogram characteristically possesses a maximum or peak intensity at the point of zero path retardation. The output of amplifier 33 is converted in generator 34 to a square wave such a shown in FIG. 2B. The square wave output of generator 34 is applied to the input of circuit 36 wherein the square wave is integrated. Thus, the output of circuit 36 will provide a zero signal when the duty cycle of the input square wave is exactly fifty percent, but any variation in the duty cycle will result in a corresponding error signal being provided at the output of error signal 36. This error signal when applied to linear ramp generator 38, changes the slope of the ramp provided by generator 38 in such a direction as to alter the velocity of mirrors 26 and 44 so as to restore the duty cycle of the output of generator 34 to precisely fifty percent. The system, therefore, constitutes a closed loop which insures that the frequency of the output of generator 34 is closely maintained at the desired value.

Detector circuit 32 provides an output signal which serves to enable gate 68 only at some time, t.sub.0, the zero path retardation peak seen by detector 28. Hence, all timing in the system can be controlled to operate from the point of zero retardation in each scanning cycle provided by interferometer 24. It will be appreciated that at the end of each excursion of mirror 26, a scanning cycle of the interferometer has been completed and that the interferometer must be reset. The controls which reset ramp generator 38 and reverse drive motor 42 and reset the output of detector 32 are not shown for the sake of clarity in exposition, but are well known and are part of the typical interferometer-spectrometer currently commercially available.

When gate 68 is enabled at t.sub.0, it passes a train of clock pulses produced by pulse generator, each pulse representing an axis crossing of the square wave produced by generator 34. A typical train of pulses is shown in timed relation in FIG. 2C. The pulse train is applied to divide-by-n circuit 72 which, therefore, provides an output pulse train, such as is shown in FIG. 2D wherein n = 6 for exemplary purposes, haing a repetition rate which is 1/n of the repetition rate of the output of gate 68. The pulse train of FIG. 2D is applied, after having been passed through delay 76, to actuate trigger circuit 66 and excite source 62 into emission. The output of excitation source 62 is shown schematically in FIG. 2E wherein the signal or flash, corresponding to the triggering pulse of FIG. 2D, rises to a maximum and and then decays to a minimum, for example, with full width at half-height of 100 microseconds. The period between pulse or initiation of the output of excitation source is, of course, 600 microseconds, corresponding to the pulse repetition rate of the output of circuit 72. This sequence of events continues with the excitation source being triggered at 600 microsecond intervals until the end of an interferometer scan in interferometer 44, whereupon the pulse train from gate 68 is terminated until the next scan has commenced and an appropriate synchronizing axis-crossing just after a zero retardation peak detection by detector 32 has occurred. Each excitation flash occurring during an interferometer scan initiates the phenomenon of interest, e.g. the photolytic decomposition of acetone in chamber 60. During the course of the decomposition, the spectral changes due to absorption of infra-red from source 64 are observed by interferometer 44 which convolves the observed spectrum with a fast Fourier transformation to produce, as well known, an interferogram. In order to provide an acceptable signal-to-noise ratio, a number of identically scanned interferograms can be coadded either through analog methods as described in U.S. Pat. No. 3,286,582 to L. Mertz, or by conversion to digital form and addition in the computer. In the example here described, the interferogram collected in one complete scan with a duration from zero retardation of 0.12 seconds, would include data derived from about 200 excitation source flashes. The number of excitation source flashes per interferometer scan, (or the number of scans per flash as the case may be) depends upon the relative length of time during which the phenomenon of interest continues (or decays) and the time period of the scan cycle, so the ratio of flashes to scans is largely a matter of choice.

Delay counter 36 is then set by setting switches 78 to interpose a one pulse period (100 microsecond) delay so that the time history of the subsequent excitation source pulses becomes as shown in FIG. 2F, i.e. is shifted by a time increment with regard to the zero retardation peak position of the interferometers. When sufficient interferograms have been obtained using the sequence of flashes of FIG. 2F, and appropriately coadded to improve signal-to-noise, the delay in counter 76 is again reset by adding another 100 microsecond delay period resulting in a time history of excitation source outputs somewhat as shown in FIG. 2G. Similarly, by altering the delay provided by counter 76 by successive 100 microsecond increments, one obtains an ordered set of excitation pulse histories such as is shown in FIGS. 2H, J and K. It will be appreciated then that for each of the excitation source histories shown in FIGS. 2E through 2K inclusive, one obtains a similarly ordered set of corresponding interferograms. These interferograms contain all of the source spectral information and the source temporal history with a two microsecond resolution, each resolution element being displaced by 100 .mu.secs from the next resolution element of 2 .mu.sec. Interferograms as produced at the output of detector 50 and amplified by amplifier 52 are, in well-known manner, sampled by sample-and-hold circuit (preferably using a 2 microsecond or less interval) and each sample is converted by analog-to-digital converter 54 to digital form for storage as an ordered set in computer 56.

Preferably, delay 70 is adjustable by 0.5 .mu.sec increments to fine tune by interposing a delay in actuating sample-and-hold circuit by the 100 .mu.sec period pulse train from gate 68. This serves to permit sampling of data to be delayed, relative to triggering of excitation source 62, to match or compensate for the usual rise time of the phenomenon in response to excitation.

From the data thus provided and stored in computer 56, one however can look at the spectrum of material in sample chamber 60 within a two microsecond resolution range or time domain. For example, if one wishes to look at the nature of the spectrum in the zero-100 microsecond time domain, one takes the data moieties or information taken during the first, seventh, thirteenth, etc., resolution elements (each of two microsecond duration) from the first interferogram corresponding to the excitation due to the excitation source history shown in FIG. 2E; the data moieties from the second, eighth, fourteenth, etc., resolution elements of the interferogram next in order and corresponding to the source history shown in FIG. 2F; the information taken during third, ninth, fifteenth, etc. resolution elements of the interferograms third in order and corresponding to the excitation source history of FIG. 2G, etc. until all stored interferograms have been sampled, and construct a new or synthetic interferogram in which each of the data moieties are placed in sequence according to the order of the original interferograms in the set. The software sorting routine needed to construct a synthetic interferogram corresponding to one time-resolution element can be constructed in the following manner, using a notation in which a letter in parentheses identifies the original interferogram by the letter caption of the excitation source history of FIG. 2, and the number in the parentheses is the ordinal value of t.sub.o from the selected time resolution element in units of 100 microseconds. For example, the notation for the temporal resolution element at 400 .mu.secs after t.sub.0 in the interferogram, corresponding to the temporal source history shown in FIG. 2G would be (G,4). Thus, synthetic interferogram for the first 100 microsecond interval of the original interferograms would be constructed by placing in sequence the data corresponding to the following (E1) (F2) (G,3), (H,4), (J,5), (K,6), (E,7), (F,8), (G,9), (H,10), (J,11), (K,12), etc. A formal software program for effecting the foregoing in a Data General 2/10 computer is attached to copending application Ser. No. 760,701 earlier identified.

Once an interferogram has been synthesized and stored again in the computer, the latter is preferably programmed to perform the inverse transformation on the synthetic interferogram to obtain the information, such as the spectrum, as it was observed during the time interval or resolution element to which the synthetic interferogram corresponds. The programs required to perform a fast Fourier transformation by digital computer, such as the Cooley-Tukey algorithm are well known in the art. Alternatively, in place of a digital computer, one can use an analog system such as heterodyne wave analyzer to perform the desired inverse transformation.

The above detailed invention was used to investigate ultraviolet photolysis of a number of materials, particularly acetone and acetaldehyde. Using the flash lamp hereinbefore described as source 62, one obtained quarter joule peak intensity, 10 .mu.sec full width half-maximum light flashes. The flash lamp operated at 250 flashes per second. A series of interferograms were taken and synthetic interferograms were formed and inversely transformed. The various time-dependent spectra are shown in FIG. 3, each representing a 2 .mu.sec interval, 400 .mu.secs apart, each identified by the time in microseconds from t.sub.o. The bottom spectrum in FIG. 3 however is a single beam spectrum of acetone (so labeled) with no UV exposure.

The time dependence of spectral features in FIG. 3 is obvious. The sampling interferometer was not purged, therefore the atmospheric CO.sub.2 feature is present in each spectrum at 2349cm.sup.-1. Photodecomposition of acetone produces CO with a band origin at 2149cm.sup.-1 superimposed upon the acetone band.

The spectral feature with a band origin at 3138cm.sup.-1 demonstrates the utility of the invention. This sequence of experiments was undertaken to study the reaction as it occurred in the well known dissociation scheme

several unexpected features were observed. The spectral feature at 3138cm.sup.-1 which has been tentatively identified as due to ketene absorption, forms after the UV flash, increases in concentration until 3.24 milliseconds, and disappears in the next 0.40 millisecond.

Other spectral features between 2500 and 2800 cm.sup.-1 appear in emission 40 microseconds after the UV flash. By 1.24 milliseconds this system is absorbing and at 3.64 milliseconds the system is once again emitting.

A similar series of spectra shown in FIG. 4 (compared to the spectrum taken without UV exposure at the bottom of FIG. 4) were derived from acetaldehyde UV photolysis according to the present invention. The very substantial changes occurring between 30 .mu.sec and 430 .mu.sec following UV exposure can readily be observed.

In the alternative form of the device of FIG. 1, as shown in FIG. 5, like parts are indicated with like numerals. Thus, the device of FIG. 5 includes the same interferometric means comprising the same parts as shown in FIG. 1, the output of both pulse generator 67 and of detector circuit 32 comprising the input to AND gate 68. The output of the latter however, is only connected to the input of divider 72.

The circuit of FIG. 5 also includes a typical settable delay means such as counter 76, the count in which is controlled or selected by manually operable setting switch 78. The output of delay means 76 is connected to the input of trigger circuit 66. The output of counter 76 however is also coupled as the input to delay circuit 70. The output of delay circuit 70 is connected, as in the embodiment of FIG. 1, to the reset terminal sample-and-hold circuit 74.

The operation of the device of FIG. 5 provides in a similar manner an output from gate 68 similar to that of the device of FIG. 1, so that as gate 68 is enabled at t.sub.0, the train of clock pulses from generator 67, as shown in FIG. 6A, is applied to divider circuit 72. The latter, as in the device of FIG. 1, provides the same pulse train (shown in FIG. 6B) which is applied, after being passed through settable delay circuit 76, to activate trigger circuit 66 and thus excite source 62 into emission as shown in FIG. 6C. The same pulse train from delay circuit 76 is also however applied through delay circuit 70 to the reset terminal of sample-and-hold circuit 74 (or alternatively to actuate A-D converter 54).

As in the system of FIG. 1, the number of excitation flashes (a consequent emissions from chamber 60) per interferometer scan depends on the number of excitation pulses applied to source 62 by circuit 76 during each scan. Circuit 76 selectively establishes the relative phase between the scan cycle and the excitation pulse train in FIG. 6B in accordance with the setting of switches 78. However, the application of the same pulse train, each pulse being delayed by a predetermined interval .DELTA.t in delay circuit 70 to either circuit 74 or A-D convertor 54 causes sampling of each of the emissions from chamber 60 to occur only once (typically over a 2.mu.sec sampling window) in the decay curve at some point in time, .DELTA.t, after initiation of the emission, quite unlike the system of FIG. 1 where sampling occurs much more frequently during the decay of each emmission. In order to permit one to select .DELTA.t, delay 70 in FIG. 5 is preferably a settable delay such as delay 76 in FIG. 1. Hence one can obtain sampling at a selected point in time in each life time of the multiplicity of emmissions observed, for a given retardation, and by coadding the samplings in known manner as hereinbefore noted, above the signal-to-noise ratio of that time sample taken at the specified retardation and time interval .DELTA.t.

As each set of emission curves is successively time-shifted by a time increment established by delay circuit 76 with regard to the zero retardation peak position of the interferometers, the sampling point remains the same with respect to initiation of the excitation curve, but shifts by that same time increment with regard to the zero retardation peak. Hence, the successive sets of samples, (each set representing a summation of samples taken at a selected retardation but at the same point in time following initiation of the emission phenomenon of interest) can simply be ordered in time to synthesize a single interferogram, which when inversely transformed as hereinbefore noted, yields the desired spectrum at that point in time in the occurrance of the emission phenomenon of interest.

A formal software program for effecting the foregoing operation of the embodiment of FIG. 5 in a Data General 2/10 computer is attached hereto as Appendix A.

The system of FIG. 5 thus simply yields one interferogram representing the spectrum of the phenomenon of interest at a time .DELTA.t after initiation of the phenomenon of interest, whereas the system of FIG. 1 produces a plurality of different timed spectra. Where only a single time spectrum is desired so that the other spectra obtained for the device of FIG. 1 are superfluous, the system of FIG. 5 will then be useful to avoid obtaining undesired or redundant data and therefore offers substantial time economy and particularly reduces data storage requirement.

Since certain changes may be made in the above apparatus and process without departing from the scope of the invention herein involved, it is intended that all matter contained in the above description or shown in the accompanying drawing shall be interpreted as illustrative and not in a limiting sense. ##SPC1## ##SPC2## ##SPC3## ##SPC4## ##SPC5## ##SPC6##