GB2295227A - Classifying diamonds - Google Patents
Classifying diamonds Download PDFInfo
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- GB2295227A GB2295227A GB9601274A GB9601274A GB2295227A GB 2295227 A GB2295227 A GB 2295227A GB 9601274 A GB9601274 A GB 9601274A GB 9601274 A GB9601274 A GB 9601274A GB 2295227 A GB2295227 A GB 2295227A
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- G—PHYSICS
- G01—MEASURING; TESTING
- G01N—INVESTIGATING OR ANALYSING MATERIALS BY DETERMINING THEIR CHEMICAL OR PHYSICAL PROPERTIES
- G01N21/00—Investigating or analysing materials by the use of optical means, i.e. using sub-millimetre waves, infrared, visible or ultraviolet light
- G01N21/84—Systems specially adapted for particular applications
- G01N21/87—Investigating jewels
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- Health & Medical Sciences (AREA)
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- General Physics & Mathematics (AREA)
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- Investigating Materials By The Use Of Optical Means Adapted For Particular Applications (AREA)
- Investigating, Analyzing Materials By Fluorescence Or Luminescence (AREA)
Abstract
In order to classify a diamond as natural or synthetic, a first signal is derived dependent upon the intensity of ultra-violet radiation transmitted by the diamond at 254nm, and a second signal is derived dependent upon the intensity of radiation transmitted by the diamond at 365nm and the diamond is classified as being definitely natural, eg type IaA or IaAB, if the first signal is substantially less than the second signal. UV light of the two wavelengths may be transmitted to and from a diamond using a rotatable mirror having opposite sides of different wavelength selective reflectivity, or by fibre optics and a rotatable filter wheel. The light emitted by the source may be measured directly at the two wavelengths using the same detector to compensate for changes in the source. <IMAGE>
Description
"METHOD AND APPARATUS FOR CLASSIFYING DIAMONDS"
Background of the Invention
This invention relates to a method and apparatus for examining objects by irradiating them with radiation and analysing the transmitted or emitted radiation. The invention also relates to a method and apparatus for classifying diamonds.
Normally, apparatus for examining objects using radiation comprises a source, which may be a laser of a particular wavelength or a broad-band illuminator such as a tungsten lamp, means for controllably exposing the object to the radiation and means for collecting radiation transmitted or emitted by the object. The transmitted or emitted radiation may be filtered to exclude the illuminating wavelength or to transmit a single wavelength of interest, the radiation passed by the filter being passed to a detector.
Such an apparatus may be used for examining diamonds, the information obtained depending on the wavelength of radiation studied.
It is desired to provide a method and apparatus for examining objects in which the intensity of the irradiating radiation may be measured, the path for measuring the irradiating radiation being as similar as possible to the path of the radiation to the object.
Furthermore, it is desired to minimise the number of parts required and to simplify the apparatus generally.
The Invention
The first aspect of the invention provides apparatus for and a method of examining an object, as set forth in
Claim 1, 16, 25 or 26. Preferred features of the invention are set out in Claims 2 to 15 and 17 to 24.
The second aspect of the invention provides a method of and apparatus for classifying a diamond as set out in
Claim 27, 32, 37 or 38, preferred and/or optional features of the method and apparatus being set out in
Claims 28 to 31 and 33 to 36.
The method and apparatus of the first aspect of the invention allow the intensity of radiation used to irradiate the object to be detected. Accordingly, temperature variations or other variations in the spectrum of the radiation source can be allowed for when interpreting the results. The apparatus can be small and simple. The same reflective member is used in the path of radiation from the sample to the detector and the source to the detector.
In the second position of the reflective member, a signal can be produced dependent upon the intensity of light which is reflected by the object, transmitted by the object, reflected through the object or emitted by the object by luminescence.
The radiation path from the source to the reflective member, from the reflective member to the object or from the reflective member to the detector is preferably as simple as possible, involving the smallest number of optical elements, to reduce the amount of radiation lost at each optical element. However, any radiation path may be used and may comprise a plurality of reflective devices. The reflective member may comprise a plurality of components but the change from the first position to the second position is achieved in this case substantially by changing the position of the reflective member as a whole or as a unit.
For simplicity, only one reflective member should be used. This is possible, because the apparatus can be set up such that radiation directed to the object and (a portion of) the radiation emanating from the object intersect the same reflective member. Preferably, the path of irradiating radiation is coincident with the path of radiation emanating from the object which intersects the reflective member. In this case, a beam splitter may be used to direct light to the detector.
Using the beam splitter allows the apparatus to be set up very simply, as it uses the principle of reversability of light. Whatever path the irradiating radiation takes (reflected back by the reflective member or reflected onto the sample), reflected radiation must be able to travel back along the path of the irradiating radiation. It will then be internipted by the beam splitter and so directed to the detector.
The beam splitter is preferably placed before the reflective member in the path of radiation coming from a source, the radiation coming from the source not being directed to the detector by the beam splitter. In this configuration, the first position of the reflective member may correspond to the reflective member being normal to the direction of radiation from the source so that the radiation -is reflected back onto the beam splitter which will then deflect the beam of radiation to the detector.
Other radiation paths may be chosen if necessary, for example a further mirror may be provided to reflect radiation back to the reflective means when in the first position.
In the simplest arrangement, the reflective member is moved and the input beam and the detector means are stationary with respect to one another. However, it would be possible to keep the beam of input radiation stationary with respect to the reflective means and to move the two parts together with respect to the detector.
The detector is preferably a photomultiplier tube, but may be any convenient form of radiation detecting means. Preferably, the detector gives a signal dependent upon the intensity of light incident upon it.
The reflective member can be mounted for rotation about an axis. This allows it to be flipped or moved quickly between the first and second position. It also facilitates taking a large number of measurements using the apparatus, by rotating the reflective member and cycling through the positions at great speed.
A polychromatic or broad band radiation source can be used easily with the present invention, which is cheaper than a laser.
The reflective member is preferably a wavelength selective mirror. This allows the apparatus to be particularly simple because a single part of the apparatus is used to selectively direct radiation in different paths and to select the radiation directed.
Preferably, two or more wavelengths may be measured by providing a second wavelength selective, reflective surface on the reflective member, for instance on the reverse side. A wavelength selective mirror having two separate wavelength selective mirrors back to back or two separate wavelength selective mirrors mounted at different positions on a rotating mount may be used.
In order to study the intensity of radiation transmitted by the object at the input wavelength, the object may be placed in an irradiation zone comprising further reflective means for reflecting radiation transmitted by the object back in the direction of the input radiation back to the reflective member. For example, an integrating sphere may be used. If the object is a cut brilliant diamond, reflective means are not required.
The radiation is input through the table of the diamond and the diamond is cut such that a large proportion of light entering the diamond through the table is transmitted by the diamond and reflected out through the table.
The second aspect of the invention allows the different ultra-violet absorption characteristics of different types of diamond (e. g. type IaAB, type II etc. ) to be used to classify a given diamond. All diamonds show strong absorption of short wave ultra-violet radiation at wavelengths less than a certain cut-off wavelength which varies from type to type.
Below the cut-off wavelength, the diamond effectively becomes opaque to the radiation.
In the second aspect of the invention, a diamond may be classified as belonging to one of two types, which are distinguished by their absorption cut-off wavelengths.
A measurement of the fraction of incident radiation absorbed (or, equally, transmitted) is made at a value between the two cut-off wavelengths. The diamond will either show very strong absorption (if it belongs to the type whose cut-off wavelength is higher than the test wavelength) or moderate absorption (if the cut-off wavelength is less than the test wavelength).
The measurement of the absorption at a wavelength between the two cut-off wavelengths should be normalised to allow for the size of the diamond. Any suitable normalising means may be used, for example a signal may be derived or input based upon the size of the diamond.
The first signal can be corrected by dividing it by the size signal.
Preferably, a further measurement should also be made at a further ultra-violet wavelength at which all types of diamond are likely to show only moderate absorption in order to provide a signal dependent upon the size of the object as a size reference for the signal.
Preferably, the first class of diamonds comprises diamonds of type IaAB which show strong absorption below about 290nm. The second class may comprise all other types of diamond, which will have strong absorptions below about 225nm. The test measurement is made at a value between 225 and 290nm and the further measurement is taken at a wavelength greater than 290nm.
Preferably, a mercury lamp is used to produce the ultra-violet radiation. Radiation produced by a mercury lamp has strong bands at 254nm and 365nm. These clearly fit the requirements for test and further wavelengths set out above. Thus, using a single source, both the test and further wavelengths may be produced.
Preferably, the second aspect of the invention is used with the first aspect of the invention. Preferably, a wavelength selective mirror having two wavelength selective faces is provided, for selecting the 254nm band and 365nm -band respectively. Radiation is fed through the table of the diamond (if it is a brilliant cut diamond) and a substantial quantity of radiation entering the diamond will be reflected through the diamond and transmitted through the table of the diamond. This transmitted radiation is directed by the reflective member to the detector.
The invention will be further described with reference to the accompanying drawings, in which:
Brief Description of the Drawings
Figure 1 shows the absorbance of ultra-violet radiation of various wavelengths for different types of diamond;
Figure 2 shows an apparatus for examining a diamond according to the second aspect of the invention;
Figure 3 shows a further embodiment of apparatus for examining a diamond according to the second aspect of the invention; and
Figure 4 shows an apparatus for examining a diamond according to the first aspect of the invention.
Detailed Description of the Drawings
Diamonds may be classified according to spectroscopic properties. The different types of diamond have their origins in different forms of impurities, which occur in small concentration in the crystal structure. The following classification is commonly used.
Type I - this general type class is defined as the class of diamonds which have a measureable defect induced infra-red absorption in the one-phonon region (below 1332cm 1). This general class type is divided into:
Type Ib - which show an optical absorption at about 600nm continuing with increasing strength into the longwave ultra-violet region due to single nitrogen atoms substituted for single carbon atoms at random throughout the crystal lattice of the diamond. This gives rise to the so-called canary yellow colour shown by some diamonds. Type Ib diamonds represent a non-equilibrated form of diamond. Diamonds are formed at conditions of very high temperature and pressure and if the diamond is maintained at these conditions, impurity nitrogen atoms will tend to aggregate.Natural diamonds are believed to have remained at equilibrating conditions for geologically significant periods of time and accordinc,ly type Ib diamonds are rare in nature. On the other hand, synthetic diamonds are not maintained at equilibrating conditions and accordingly most synthetic diamonds are type Ib.
Type Ia - this class comprises diamonds in which the nitrogen has migrated to form more complex defects.
There are two principal forms of nitrogen defect which are found in type Ia diamonds, the A form and B form.
The A form comprises pairs of nitrogen atoms on nearest-neighbour substitutional sites. The B form of nitrogen is believed to comprise a complex of four substitutional nitrogen atoms surrounding a vacancy.
The ratio of the concentration of A type defects to B type defects varies continuously, the extreme ends of the sequence being labelled type IaA and type IaB. Pure type IaB diamonds are very rare.
Type A centres are associated with a relatively high ultra-violet absorption at wavelengths below about 3OOnm.
As type A centres are believed to be the result of remaining at equilibrating conditions for a considerable period of time, synthetic diamonds almost never have type A centres. Most naturally occurring diamonds contain both A and B centres and are classified as
IaAB. They retain the strong absorption at wavelengths below 300nm.
Type IIa - This class comprises diamonds in which nitrogen is only present in trace amounts, of the order of lppm. This near absence of nitrogen in diamonds rarely occurs in nature but can be assured in the production of synthetic diamonds.
Type IIb - This is a very rare class of semi-conducting diamonds which contain trace amounts of substitutional boron. Type lIb diamonds are generally natural, but synthetic diamonds having added boron can be produced.
Accordingly, type Ib, IIa and lib diamonds may be produced synthetically. It is, however, almost impossible to produce type IaA, type IaB or type IaAB diamonds synthetically. All of the latter three types of diamonds encountered would be most likely to be natural.
Figure 1 shows a series of graphs of absorbance (absorption coefficient per unit path length) in arbitrary units, for a set of typical stones of different class.
All the curves show a steep region at lower wavelengths and a flat region at higher wavelengths, with a relatively sharp junction.
Substantial absorption may be thought of as absorption substantially greater than that found in the flat region, for example 20 times greater, or more.
The invention provides a method of distinguishing natural from synthetic diamonds based upon the short wave ultra violet radiation absorption characteristics.
This can be done by identifying the increased absorption below 300nm associated with A centres. As shown in
Figure 1, the absorption of ultra violet by all the other major types of diamond does not increase much at wavelengths down to about 225nm, which is a characteristic absorption of all types of diamond. The high absorption associated with type A centres below 300nm may be detected by comparing a measurement of the ultra-violet absorption at a wavelength above 300nm with the absorption at a wavelength below 300nm but greater than the intrinsic diamond absorption at 225nm. As can be seen from figure 1, the ratio of these two measurements will be in the region 1: 1 or 2 for diamonds of type IaB, IIA and IIb.However, diamonds of type IaA will have a ratio in the region of 1: 20 or 1: 100 or more.
This technique will identify type IaA diamonds and IaAB diamonds, which represent the vast majority of all natural diamonds. Natural diamonds of type IaB will fail the test. However, the very small occurrence of laB diamonds in nature renders this defect of minor importance compared with the advantages to be obtained in producing an apparatus which can positively identify the vast majority of natural diamonds. In total, 95% of natural diamonds will pass the test and only 5% will be rejected. These latter can be subjected to other tests.
Figure 2 shows an apparatus for examining diamonds, according to the method of the invention described in relation to Figure 1 above. This apparatus comprises a radiation source 1 which is suitably a mercury vapour lamp. A mercury vapour lamp produces two strong bands of ultra-violet radiation at 365nm and 254nm. These two wavelengths are suitable for the method of the invention described in relation to Figure 1 above.
Radiation from the source 1 is reflected by mirror 2 through filter wheel 3. The filter wheel 3 has a number of apertures 4 which may also be provided with narrow band pass filters for passing radiation at 365nm or 254nm to the diamond. All other wavelengths are blocked by the filter so that the quantity of energy directed onto diamond 5 is not too high. The filter wheel 3 is rotated by motor 6 to present different filters 4 in succession. Radiation passed by filter 4 is transmitted by fibre optic line 7 to the diamond 5.
Preferably, radiation is directed into the table of a cut diamond 5. If the diamond has a brilliant cut, a large quantity of the radiation incident on the table will be reflected out through the table. A second fibre optic line 8 collects radiation transmitted through the diamond in this manner.
A second filter wheel 9 comprises filters 10 for passing radiation at 365nm or 254nm. The second filter wheel 9 is altered by motor 11 so that the radiation passed by filter 10 is of the same wavelength as the radiation directed to diamond 5 by filter 4.
The second set of filters is required to exclude radiation produced by fluorescence etc, which would otherwise give an incorrect result. The radiation passed is detected by suitable means 12 such as a photomultiplier tube. The signal produced by the photomultiplier tube 12 is amplified at 13 to provide a signal for a microprocessor 14.
The microprocessor 14 can control the positions of the filter wheels 3 and 9 via motors 6 and 11 and thereby measure the radiation transmitted at both of the wavelengths of interest. The intensities of radiation transmitted at wavelengths of interest are then compared to decide whether the diamond is natural or synthetic.
The result may be displayed on a display means 15.
The ratio of the intensities of radiation transmitted at the two wavelengths may be taken, the diamond being classified as natural if the ratio of radiation absorbed at 254nm to that absorbed at 365nm is greater than 20: 1, preferably greater than 50: 1, most preferably greater than 100: 1.
Figure 3 shows further apparatus for classifying a diamond according to the method described in relation to figure 1 above. In this apparatus, there is no primary filter between the source 1 and diamond 5, radiation being transmitted from the source 1 via fibre optic 16 to the diamond. Radiation transmitted by the diamond is collected by fibre optic 17 and passed through a filter 18 which is a narrow band pass filter passing radiation at a wavelength of 254nm or 365nm. The filter 18 is mounted in a filter wheel 19 for quick change between filters of the different wavelengths. The filter wheel 19 is rotated by motor 20. Radiation passed by filter 18 is collected by photomultiplier tube 21, amplified at 22 and processed by a microprocessor 23.
In order to provide information about the intensity of radiation generated by source 1, which may vary with the mains voltage applied and thus produce errors, a reference line 24 takes radiation directly from the source 1. The microprocessor 23 may control the position of the filter wheel 19 to present a filter 26 to position 27 to pass radiation of the wavelength of interest (254nm or 365nm) from fibre optic 24 to a mirror and beam combiner system 28 whilst blocking radiation from fibre optic 17. The radiation transmitted by filter 26 is then passed to the photomultiplier tube 21 for providing a signal representative of the illumination intensity.
Figure 4 shows yet further apparatus for putting the method described in relation to figure 1 above into practice, using the idea of the second aspect of the invention.
In this apparatus, the neans for irradiating an object comprises a source 1 directing radiation through lens 29 and beam-splitting mirror 30 on to a reflective member in the form of a wavelength selective mirror 31. The wavelength selective mirror 31 comprises a wavelength selective surface 31a for reflecting radiation of a wavelength at 254r.m, and a separate wavelength-selective face surface 31b for reflecting radiation at a wavelength of 365nm on the opposite side of the mirror.
The wavelength selective mirror 31 is rotated so that the different faces 31a and 31b of the mirror 31 are presented to the beam of radiation 32 from the source 1 at different positions, defir.ed by different angles of rotation.
At a first angular position, wavelength-selective surface 31a will be normal to the beam of radiation 32, so that radiation of wavelength 254nm is reflected back to the beam splitter 30 which directs the reflected radiation to photomultiplier tube 34. The signal produced by the photomultiplier tube 34 is amplified at 35 and stored in the microprocessor 36. Thus the first angular position provides a signal representative of the intensity of radiation produced by illuminating means 1 at 254nm.
As the mirror rotates, it reaches a second angular position at which surface 31a reflects radiation of the selected wavelength (254nm) from source 1 onto the table of diamond 33. The radiation interacts with the diamond and a substantial quantity of radiation is transmitted by the diamond and reflected out through the table of the diamond 33 back to the surface 31a. Surface 31a serves to filter out radiation of different wavelengths to 254nm emanating from the diamond (due, for example, to fluorescence) and reflects light at 254nm to the beam splitter 30 and thence to photomultiplier tube 34. Thus in the second angular position, a signal or reading is produced representative of the radiation transmitted by the diamond 33 at 254nm.An aperture (not shown) may be provided between the mirror 30 and wavelength selective mirror 31 or between wavelength selective mirror 31 and object 33 for defining the size of the beam directed to the object or to the detector.
As the mirror continues to rotate, it will present surface 31b to the beam of radiation 32, which surface selectively reflects radiation at 365nm. At a third angular position radiation of wavelength 365nm will be reflected back to beam splitter 30 and thence to photomultiplier tube 34. Thus the third angular position will provide a signal or reading representative of radiation produced by the source 1 at 365nm.
Finally, in a fourth angular position wavelength-selective surface 31b will direct light of a wavelength of 365nm onto the table of diamond 33, and will reflect radiation emanating from the diamond at a wavelength of 365nm to the beam splitter 30, so that photomultiplier tube 34 can produce a signal or reading representative of the intensity of radiation transmitted by the diamond at 365nm.
The signals or information thus provided can be stored by the microprocessor 36 and analysed as follows. The two measurements of the intensity of radiation produced by source 1 at the different wavelengths may be used to correct the measurements of intensities of radiation emanating from the diamond 33 at the respective wavelengths, to allow for changes in source temperature etc. Then the corrected readings of intensity of radiation emanating from the diamond at the two wavelengths are ratioed, and the diamond is classified in the manner described in relation to the first embodiment, above.
An angle transducer may be provided for detecting the angular position of the selective mirror 31 and giving signals to the microprocessor 36 representative of the wavelength of radiation reflected onto the diamond by the selective mirror 31
Preferably the selective mirror 31 has the 254nm selective surface 31a on the opposite surface to the 365nm selective surface 31b. However, these surfaces could be configured at an angle to each other, the only condition being that each surface will at some position provide illumination intensity information by reflecting radiation back to the beam splitter.
In the apparatus shown in Figure 4, the first and third positions correspond to reflective surfaces being normal to the beam of radiation from the source.
Alternatively, a further plane back-reflecting mirror may be provided, and the wavelength selective mirror need not be normal to the beam of radiation from the source. The back- reflecting mirror will be placed so that it is normal to the beam of radiation reflected by the wavelength selective mirror in the first position.
Equally, three or more wavelength selective mirrors could be provided for measuring the intensity of radiation transmitted by the diamond at three or more different wavelengths.
The apparatus of any of figures 2, 3 and 4 may be used in the following manner. Instead of taking a single measurement of the radiation emanating from the object at each of the wavelengths of interest and a single measurement of the illumination intensity at each of the wavelengths of interest, all four of these values may be measured in turn in a cycle which is repeated many times over. The microprocessor will store each measurement for each cycle to provide a mass of data which can be statistically analysed to provide a far more accurate reading than could be produced by a single set of measurements.
This statistical technique is of value generally in that it can cancel out random errors in the illuminating, mounting or detecting system. For example, if the diamond is loosely held in the apparatus (for example by hand) it may be vibrating, leading to errors in the orientation of the table of the diamond or the like.
Time variations in the readings can be analysed statistically by the microprocessor and readings lying outside the bulk of the data may be rejected.
Example
An apparatus was set up as shown in Figure 4. A mercury lamp capable of producing ultraviolet radiation in the band 180 to 350 nm was used. An ultraviolet transmitting lens, for example a fused silica lens as made by Comar Instruments was used. Wavelength selective mirror 31 had wavelength selective coatings 31a and 31b supplied by Tec Optics Limited. Detector 34 comprised a photomultiplier tube of the type R1414 manufactured by Hamamatsu Photonics. Display processing electronics 36 were provided.
The present invention has been described above only by way of example, and modifications can be made within the invention.
Claims (10)
1. A method of classifying a diamond as belonging to a first class comprising definitely natural diamonds or to a second class comprising diamonds which may be natural or synthetic, comprising: irradiating the diamond with ultra-violet radiation; giving a signal dependent upon the intensity of radiation transmitted by the diamond at a test wavelength lying between a first wavelength equal to the maximum wavelength at which substantial absorption occurs in the first class of diamonds and a second wavelength equal to the maximum wavelength at which substantial absorption occurs in the second class of diamonds; normalising the signal; and classifying the diamond on the basis of the normalised signal.
2. The method of Claim 1, wherein the first mentioned signal is normalised by giving a further signal dependent upon the intensity of radiation transmitted by the diamond at a further wavelength greater than the higher of the first and second wavelengths and classifying the diamond as definitely natural if the first mentioned normalised signal is substantially greater than the further signal.
3. The method of Claim 1 or 2, wherein the first class of diamonds comprises diamonds of type IaAB or IaA and the second class of diamonds comprises diamonds not of type IaAB nor of type laA.
4. The method of Claim 2 or 3, wherein the further wavelength is the 365nm band of a mercury lamp, and the test wavelength is the 254nm band of a mercury lamp.
5. Apparatus for classifying a diamond as belonging to a first class comprising definitely natural diamonds or to a second class comprising diamonds which may be natural or synthetic, comprising:
means for irradiating the diamond with ultra-violet radiation;
means for giving a signal dependent upon the intensity of ultra-violet radiation transmitted at a test wavelength lying between a first wavelength equal to the maximum wavelength at which substantial absorbtion occurs in the first class of diamonds and a second wavelength equal to the maximum wavelength at which substantial absorption occurs in the second class of diamonds;
means for normalising the signal; and
means for giving a signal for classifying the diamond on the basis of the normalised signal.
6. The apparatus of Claim 5, wherein the means for normalising the first mentioned signal comprise means for giving a further signal dependent upon the intensity of radiation transmitted at a further wavelength greater than the higher of the first and second wavelengths.
7. The apparatus of Claim 6, wherein the further wavelength is the 365nm band of a mercury lamp and the test wavelength is the 254nm band of a mercury lamp.
8. The apparatus of Claim 6 or 7, wherein the ratio of the first mentioned signal to the further signal is taken and the object is classified as belonging to the first class if the ratio of the first mentioned signal to the further signal is greater than 5.
9. A method of classifying a diamond, substantially as herein described with reference to and as shown in the accompanying drawings.
10. Apparatus for classifying a diamond, substantially as herein described with reference to and as shown in the accompanying drawings.
10. Apparatus for classifying a diamond, substantially as herein described with reference to and as shown in the accompanying drawings.
Amendments to the claims have been filed as follows 1. A method of classifying a diamond as belonging to a first class comprising definitely natural diamonds or to a second class comprising diamonds which may be natural or synthetic, comprising: irradiating the diamond with ultra-violet radiation; giving a signal dependent upon the intensity of radiation transmitted by the diamond at a test wavelength lying between a first wavelength equal to the maximum wavelength at which substantial absorption occurs in the first class of diamonds and a second wavelength equal to the maximum wavelength at which substantial absorption occurs in the second class of diamonds; normalising the signal; and classifying the diamond on the basis of the normalised signal.
2. The method of Claim 1, wherein the first mentioned signal is normalised by giving a further signal dependent upon the intensity of radiation transmitted by the diamond at a further wavelength greater than the higher of the first and second wavelengths and classifying the diamond as definitely natural if the signal at the test wavelength is substantially less than the further signal.
3. The method of Claim 1 or 2, wherein the first class of diamonds comprises diamonds of type IaAB or IaA and the second class of diamonds comprises diamonds not of type IaAB nor of type laA.
4. The method of Claim 2 or 3, wherein the further wavelength is the 365nm band of a mercury lamp, and the test wavelength is the 254nm band of a mercury lamp.
5. Apparatus for classifying a diamond as belonging to a first class comprising definitely natural diamonds or to a second class comprising diamonds which may be natural or synthetic, comprising:
means for irradiating the diamond with ultra-violet radiation;
means for giving a signal dependent upon the intensity of ultra-violet radiation transmitted at a test wavelength lying between a first wavelength equal to the maximum wavelength at which substantial absorption occurs in the first class of diamonds and a second wavelength equal to the maximum wavelength at which substantial absorption occurs in the second class of diamonds;
means for normalising the signal; and
means for giving a signal for classifying the diamond on the basis of the normalised signal.
6. The apparatus of Claim 5, wherein the means for normalising the first mentioned signal comprise means for giving a further signal dependent upon the intensity of radiation transmitted at a further wavelength greater than the higher of the first and second wavelengths.
7. The apparatus of Claim 6, wherein the further wavelength is the 365nm band of a mercury lamp and the test wavelength is the 254nm band of a mercury lamp.
8. The apparatus of Claim 6 or 7, wherein the ratio of the first mentioned signal to the further signal is taken and the object is classified as belonging to the first class if the first mentioned signal is less than 1/5 of the further signal.
9. A method of classifying a diamond, substantially as herein described with reference to and as shown in the accompanying drawings.
Priority Applications (1)
Application Number | Priority Date | Filing Date | Title |
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GB9601274A GB2295227B (en) | 1992-05-19 | 1993-05-19 | Method and apparatus for classifying diamonds |
Applications Claiming Priority (3)
Application Number | Priority Date | Filing Date | Title |
---|---|---|---|
GB929210674A GB9210674D0 (en) | 1992-05-19 | 1992-05-19 | Method and apparatus for examining an object |
GB9310337A GB2267147B (en) | 1992-05-19 | 1993-05-19 | Method and apparatus for examining an object |
GB9601274A GB2295227B (en) | 1992-05-19 | 1993-05-19 | Method and apparatus for classifying diamonds |
Publications (3)
Publication Number | Publication Date |
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GB9601274D0 GB9601274D0 (en) | 1996-03-27 |
GB2295227A true GB2295227A (en) | 1996-05-22 |
GB2295227B GB2295227B (en) | 1996-07-17 |
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GB9601274A Expired - Fee Related GB2295227B (en) | 1992-05-19 | 1993-05-19 | Method and apparatus for classifying diamonds |
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Cited By (3)
Publication number | Priority date | Publication date | Assignee | Title |
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EP1657544A1 (en) * | 2004-11-10 | 2006-05-17 | Wetenschappelijk en Technisch Onderzoekscentrum voor Diamant | Method for discerning colourless and almost colourless diamonds and arrangement for carrying out this method |
WO2015007873A1 (en) * | 2013-07-18 | 2015-01-22 | De Beers Centenary AG | Measuring parameters of a cut gemstone |
WO2019123383A1 (en) * | 2017-12-21 | 2019-06-27 | Università Degli Studi Di Milano - Bicocca | System and method for spectroscopy analysis of diamonds |
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GB2244329A (en) * | 1990-04-24 | 1991-11-27 | Gersan Ets | Identifying gemstone type. |
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US4291975A (en) * | 1979-10-03 | 1981-09-29 | Scientific Gem Identification, Inc. | Apparatus for determining the color characteristics of a gem |
GB2244329A (en) * | 1990-04-24 | 1991-11-27 | Gersan Ets | Identifying gemstone type. |
Cited By (8)
Publication number | Priority date | Publication date | Assignee | Title |
---|---|---|---|---|
EP1657544A1 (en) * | 2004-11-10 | 2006-05-17 | Wetenschappelijk en Technisch Onderzoekscentrum voor Diamant | Method for discerning colourless and almost colourless diamonds and arrangement for carrying out this method |
BE1016537A3 (en) * | 2004-11-10 | 2007-01-09 | Wetenschappelijk En Tech Onder | METHOD FOR DISTINCTING COLORLESS AND ALMOST COLORLESS DIAMONDS AND ARRANGEMENT FOR CARRYING OUT THIS METHOD. |
US7277161B2 (en) | 2004-11-10 | 2007-10-02 | Wetenschappelijk En Technisch Onderzoekscentrum Voor Diamant | Method for discerning colorless and near colorless diamonds and arrangement for carrying out this method |
WO2015007873A1 (en) * | 2013-07-18 | 2015-01-22 | De Beers Centenary AG | Measuring parameters of a cut gemstone |
CN105593668A (en) * | 2013-07-18 | 2016-05-18 | 戴比尔斯英国有限公司 | Measuring parameters of a cut gemstone |
US9958398B2 (en) | 2013-07-18 | 2018-05-01 | De Beers Uk Ltd. | Measuring parameters of a cut gemstone |
WO2019123383A1 (en) * | 2017-12-21 | 2019-06-27 | Università Degli Studi Di Milano - Bicocca | System and method for spectroscopy analysis of diamonds |
US11906437B2 (en) | 2017-12-21 | 2024-02-20 | Università Degli Studi Di Milano - Bicocca | Systems and methods for spectroscopic analyses of diamonds |
Also Published As
Publication number | Publication date |
---|---|
GB9601274D0 (en) | 1996-03-27 |
GB2295227B (en) | 1996-07-17 |
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