The present invention relates to an optical interferometer, in particular to a scanning interferometer and more particularly to a scanning interferometer operating according to the Michelson principle or a principle derived there from (generally referred to in this specification as a ‘Michelson type’ interferometer).
Known scanning interferometers, such as those of the Michelson type, generally comprise two or more reflectors, such as mirrors or retro-reflectors, and a beamsplitter with at least one of the reflectors being arranged to be reciprocally movable. An observation beam, generally consisting of radiation in a wavelength region of interest either before or after its interaction with a sample material, enters the interferometer and strikes the beamsplitter. This beam is split into essentially two equal parts at the beamsplitter. A first beam is reflected by the beamsplitter and travels along a first ‘arm’ to the first reflector. A second beam passes through the beamsplitter and travels along a second ‘arm’ to the second reflector.
The first beam is reflected by the first reflector, passes back along the first arm, through the beamsplitter, and continues to a detector. Meanwhile, the second beam is reflected by the second reflector, passes back along the second arm, returns to the beamsplitter, and is also reflected to the detector. An interference pattern (interferogram) is then recorded by the detector as the one or more reflectors are moved to create cyclic excursions of the related optical path and hence a cyclic optical path length difference between the first and the second beams. As a result of this interference each wavelength in the observation beam is modulated at a different frequency. Spectral information may then be extracted from the interferogram by numerically performing a Fourier transform (FT).
In the recording of an interferogram, particularly when using the so-called Fast FT technique, the sampling at exact equidistant positions of the moving reflector is critical for avoiding error. However the movement of the reflector with sufficiently low variation requires the use of very expensive actuators, and therefore it has become practice in FT spectroscopy to use a source of radiation of known wavelength, such as a laser, to generate a reference beam in a reference FT interferometer. This reference FT interferometer operates in parallel to the FT interferometer used for monitoring the observation beam (the principle interferometer) in order to generate a reference interferogram. The wavelength of the reference source is accurately known and the parallel operation means that the movable reflector of the reference FT interferometer is made to move in a known relationship with that of the principle FT interferometer. Features, such as zero crossing positions, of the reference interferogram can therefore be employed to accurately determine the incremental displacement and/or velocity of the movable reflector in the principle FT interferometer. Thus the sampling frequency for the observed radiation may be accurately determined. However, the use of a separate reference interferometer which is mechanically coupled to the principle FT interferometer adds considerably to the cost and the complexity of the system. It has therefore become practice to obtain the reference interferogram directly through the principle interferometer by employing a reference source and associated detector chosen to operate at a wavelength outside and below the wavelength region of the radiation constituting the observation beam. It is common practice to select a reference source which emits at a wavelength satisfying the Nyquist sampling criterion, requiring the sampling frequency to be at least twice the frequency of the observed signal.
In the known interferometers of the type in which the reference interferogram is obtained in the principle interferometer the optical path for the observation beam through the interferometer and the optical path for the reference beam through the interferometer include the same optical components. However the actual optical paths through these components may be substantially different. This results in each beam interacting with a different portion of these optical components. This has the disadvantage that the optical components must be made large enough to accommodate the two distinct optical paths. Moreover, the reference beam typically interacts with the edges of the optical components which, for movable components at least, could mean that there is a difference between the movement monitored by the reference beam and that experienced by the observation beam.
According to one aspect of the present invention there is provided an optical interferometer as described in and characterised by the present Claim 1. By using a suitably disposed dichroic filter both the optical path for the observation beam and that for the reference beam are collocated, usefully in co-location. This has the advantage that both beams interact with substantially the same portions of the optical components which are common to both the observation beam and the reference beam. This results in the possibility to reduce the size of these optical components and hence the opportunity to provide a more compact interferometer. Moreover, the reference beam more accurately represents any changes in the light path through these components which may be experienced by the observation beam.
These and other advantages will become apparent from a consideration of the following description of exemplary embodiments made with reference to the drawings of the accompanying figures, of which:
Referring now to
An observation beam 18 is caused to traverse a first path 20 which divides at the beamsplitter 6 along the first 1 and the second 2 arms to be reflected by respectively the fixed mirror 8 and the movable mirror 10. In the present example a suitable lens 22 generates a parallel observation beam 18 which passes into the interferometer 4 through an entrance aperture 24 in the housing 16 to traverse the first optical path 20. Other means of introducing the observation beam 18 into the interferometer 4, such as for example an arrangement including a fibre optical guide, will be well known to the person skilled in the art.
Also illustrated as part of the known scanning interferometer 4 of
In the known scanning interferometer 4 the reference beam 30 is caused to traverse a second optical path 32 which includes the beamsplitter 6 and the fixed 8 and movable 10 mirrors. This second optical path 32 is essentially parallel to but substantially laterally displaced from the first optical path 20.
In use the observation beam 18 traverses the first optical path 20 to be split into two substantially identical partial beams. One partial beam will traverse that portion of the first optical path 20 along the first arm 1 to be reflected from the fixed mirror 8 to traverse the same first arm 1 towards the beamsplitter 6. The other partial beam will traverse that portion of the first optical path 20 extending along the second arm 2 to be reflected from the movable mirror 10 back along the same second arm 2 towards the beamsplitter 6. The partial beams recombine at the beamsplitter 6 and traverse a common portion 3 of the first optical path 20 towards a detector (not shown). Simultaneously, the reference beam 30 traverses the second optical path 32 and is similarly split into two substantially identical partial beams. One partial beam will traverse that portion of the second optical path 32 which extends along the first arm 1 and the other partial beam will traverse that portion of the second optical path 32 which extends along the second arm 2. The second optical path 32 travelled by the reference beam 30 between the beamsplitter 6 and the two mirrors 8,10 is substantially parallel to but significantly laterally displaced from first optical path 20 traversed by the partial beams originating from the observation beam 18. Upon reflection from the corresponding mirrors 8,10 the two partial beams derived from the reference beam 30 will recombine at the beamsplitter 6 to traverse a common portion 38 of the second optical path 32 towards the detector 28. The interference pattern (interferogram) that is registered at the detector 28 and which is consequent on the reciprocating movement of the mirror 10 may then be employed to monitor the movement of that mirror 10.
A dichroic filter 80′ is often also a component of the known interferometer 4 where it is employed to prevent shorter wavelengths (that is wavelengths shorter than those of the observation beam 18) from reaching the detector (not shown). Such shorter wavelengths may be generated by stray ambient light reaching the entrance aperture 24 of the interferometer 4. In order to achieve this filtering the filter 80′ is located in the first optical path 20 for the observation beam 18 either before or after the beamsplitter 6. Suitable positions of the filter 80′ are illustrated by the broken lined constructions in
Considering now an exemplary embodiment of a Michelson type interferometer 40 according to the present invention which is illustrated in
As with the known interferometer of
Similar to the known interferometer 4, the exemplary interferometer 40 according to the present invention also comprises a reference radiation source 70 and complimentary detector 72 arrangement. Different to the known interferometer 4, the interferometer 40 is configured such that a beam of reference radiation 76 will traverse a second optical path 78 that intersects the first optical path 56 for the observation beam 52 at a location (generally indicated by L) that, in the present embodiment, is before the beamsplitter 42.
A dichroic filter 80 is included as an element of the interferometer 40 and is located in the region of the location of the intersection L to interact with both the observation beam 52 and the reference beam 76 and thereby collocate associated first 56 and second 78 optical paths in a common direction towards the beamsplitter 6. This results in the first 56 and the second 78 optical paths intersecting substantially the same regions of the optical elements 42,46,48 which delimit the first 50 and the second 60 arms of the interferometer 40. This has an advantage that these optical elements can be reduced in size as compared with those of the known interferometer of
The dichroic filter 80 is selected to, in use, permit the transmission of one or other of the observation beam 52 and the reference beam 76 (in the present embodiment the observation beam 52) substantially unhindered whilst reflecting the other (here the reference beam 76) beam.
According to the exemplary embodiment of
The optical path 78 for the reference beam 76 through the interferometer of
An example of such a compact construction of the interferometer 40 is illustrated in
In the present embodiment two bore holes 92, 94 are made at an angle, here substantially 90°, to one another and pass through the block 90. At the intersection of the two through bores 92,94 is positioned the beamsplitter 42 and compensator 44 arrangement. This beamsplitter arrangement 42,44 is to be located using a third bore 98 (illustrated by hatched line) which is provided at substantially 45° to the two through bores 92,94 and out of the plane of the figure. A fourth bore 100 is provided in the block 90 to intersect the through bore 94 at a location at which a dichroic filter (80) is to be introduced via a fifth bore 102. This fifth bore 102 intersects bores 94 and 100 at substantially 45°. The fourth bore 100 is provided to receive the mount 74 holding the reference source 70 and associated detector 72. A fixed reflector 46 and movable reflector 48 may be introduced into the associated through-bores 92, 94.
Some or all of the bore holes 92, 94, 102 may be advantageously provided with an elliptical cross-section (as illustrated by the broken line 96 with respect to the through bore 92). This ensures maximal material support for the optical and mechanical elements whilst providing minimum interference of the light beams through the interferometer which is elliptically shaped by the projection of the 45° beamsplitter arrangement 42,44.
In this arrangement the observation beam 52 enters the housing 90 via the through bore 94 at an end opposite the movable reflector 48 and intersects the beam of reference radiation 76 at substantially 90°. The dichroic filter 80 is located at this intersection and bisects the angle between the two beams 52, 76 to generate a common path for both beams 52, 76 towards the beamsplitter arrangement 42,44.
A suitable holder for optical components such as the beamsplitter arrangement 42,44 and the dichroic filter 80 of the compact interferometer illustrated in
Biasing means, here in the form of ‘pins’ 110a, 110b and 110c made from small gauge wire such as piano wire, are provided to slidably engage with and to urge the optical element in to contact with the inwardly projecting support means 108 of the holder 106. A corresponding hole, 112c say, is provided for each pin, 110c say, through the holder 106 at an angle for directing the pin 110c towards the inwardly projecting support means 108. The relatively small biasing means 110a-c as compared to that used in traditional optical mounts provides a relatively larger optical aperture of the supported optical element, allowing a smaller optical element to be employed. The strong springs provided by the pins 110a,b,c will yield low sensitivity towards vibration but, as they slidably engage with the optical element, will still allow for material response to compressional and thermal variations without distorting the optical element 80,42,44.
A further embodiment of an interferometer 120 according to the present invention is shown schematically in
As with the interferometers 4 and 40 previously described, the observation beam 152 enters the interferometer 120 to follow a first optical path 162 through the interferometer 120. The beamsplitter 124 intersects this first optical path 162 and causes two partial observation beams to each traverse an associated portion of the first optical path 162 along respective first 122 and second 128 arms of the interferometer 120. After these partial beams recombine at the beamsplitter 124 the observation beam 152 traverses a common portion 168 of the first optical path 162 towards the exit aperture 150.
The reference source 140 is, in the present embodiment, located within the interferometer 120 to generate a reference beam 166 which traverses a second optical path 164 to intersect the first optical path 162 for the observation beam 152 substantially at right angles and at a location L between the beamsplitter 124 and the exit aperture 150. The dichroic filter 138 is located in the region of the intersection L.
The filter 138 is configured to pass the observation beam 162 that is incident on a first surface 139 whilst reflecting the reference beam 166, which is also incident on the first surface 139. The filter 138 causes the reference beam 166 from the reference source 140 to traverse the second optical path 164 to the beamsplitter 124 where it then traverses the portions of the second optical path 164 that extend between the two arms 122, 128. After recombining at the beamsplitter 124 the reference radiation beam 166 traverses the second optical path 164 towards the dichroic filter 138. The filter 138 acts to reflect this reference beam 166 along a bifurcation (exaggerated in the
As will be appreciated and in common with the embodiment of the interferometer 40 according to the present invention illustrated in
Filing Document | Filing Date | Country | Kind | 371c Date |
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PCT/EP2009/055123 | 4/28/2009 | WO | 00 | 9/9/2011 |