ALIGNMENT MEANS FOR A LIGHT SOURCE EMITTING INVISIBLE LASER LIGHT

Abstract: An alignment means for a light source (10) emitting invisible laser light intended, for, example, as a guide beam in a laser alignment agent. The means includes a monocular (5,6), a reflecting prism (4) for deflecting part of the emitted laser light and reflecting it to the objective (5) of the monocular, and an image converter (19) for generating a visible image of the reflected laser light. The problem with a heavily deteriorated monocular image due to the image converter is avoided by the converter (19) being spaced from the optical axis (7) of the monocular and by the reflected laser light solely being taken through the image converter (19), subsequent to which the now visible laser image is superimposed on the ordinary monocular image.

Description: TECHNICAL FIELD The invention relates to an alignment means for a light source emitting invisible laser light. The means includes a monocular telescope, a reflecting prism arranged to deflect a part of the emitted laser light and reflect it to the objective of the monocular telescope, and an image converter for generating a visible image of the reflected laser light. The alignment means can be used, for example, in association with a laser alignment agent where the laser beams function as so-called guide beam. BACKGROUND ART In known apparatus of this kind the image converter is situated inside the monocular telescope, e.g. at the focal point of the light rays in the vicinity of the monocular telescope eyepiece. However, this results in that the ordinary monocular telescope image is give poor resolution and will be greenish, due to the restricted performance of the image converter with respect to resolution and spectral range. Small details at large distances will therefore merge together in the monocular telescope image. Known apparatus of this kind is described in DE 2536878. DISCLOSURE OF INVENTION The object of the present invention is to provide an alignment means of the kind mentioned in the introduction, but in which the problem with a greatly deteriorated monocular telescope image is avoided. This is achieved by the image converter being situated spaced from the optical axis of the monocular telescope and that only the reflected laser light is taken through the image converter, after which the now-visible laser image is superimposed on the ordinary monocular telescope image. The characterizing features of the invention are apparent from the claims. BRIEF DESCRIPTION OF DRAWINGS The invention will now be described in more detail below with reference to the drawings, on which Figure 1 illustrates a known alignment means, Figure 2 illustrates a first embodiment of an alignment means in accordance with the invention, Figure 3 illustrates a part of a second embodiment of an alignment means in accordance with the invention and Figure 4 illustrates a part of the means according to Figure 3 seen from one side. BEST MODES FOR CARRYING OUT THE INVENTION A known alignment means is illustrated in Figure 1. A light source 1 generates visible laser light. Transmission optics including a divergent lens 2 and a convergent lens 3 provide a parallel ray bundle, which partially impinges on a prism 4. The prism is of the type which reflects incident rays in a manner such that the reflected rays, at least practically, will be parallel to the incident rays irrespective of their angle of incidence to the prism. A so-called cube corner prism is an example of a prism having such properties. A monocular telescope with its optical axis 7 is provided with an eye piece 6 and an objective 5 and is arranged parallel to the laser rays. A part of the emitted laser beam is deflected with the aid of the prism into the monocular telescope image field and is perceived in the monocular telescope as an illuminated dot. The position of the dot in the monocular telescope image shows the direction of the laser with an accuracy solely determined by the precision of the prism. The laser and the monocular telescope thus do not need to be completely parallel. In the use of a laser emitting invisible light it is known to place an image converter at the eyepiece of the monocular telescope. In such a case the image converter is placed with its input surface in the focal plane of the monocular telescope and achieves a visible spot of the reflected laser light in the monocular telescope. As mentioned above, the ordinary monocular telescope image is deteriorated due to the image converter, in as far as the image is given poor resolution and becomes greenish, which can result in that small details cannot be distinguished. A first embodiment of an alignment means in accordance with the invention is illustrated in Figure 2. A light source 10 generates invisible laser light. The units 2-7 correspond to the units with the same numerical designations in Figure 1. The light rays in the monocular telescope are collimated by a convergent lens 12 after having passed a first focal plane 11. Visible light then passes a first 13 and a second 14 beam splitter, and is focused by a convergent lens 15 towards a second focal plane 16. The beam splitter 13 is adapted to deflect the reflected and the invisible laser light. The deflected rays are focused on the input surface of an image converter 19 with the aid of a convergent lens 17 and a reflecting member 18. The image converter is thus situated spaced from the optical axis 7 of the monocular telescope and is therefore solely passed through by the laser light. The light rays from the output surface of the image converter, these rays representing the now-visible and greenish image of the laser spot, are reflected by a reflecting member 20, collimated by a convergent lens 21 and are then incident on the beam splitter 14. The reflecting members 18 and 20 may be such as prisms or mirrors. The beam splitter 14 is adapted to pass the visible light through from the beam splitter 13 and deflect the light from the image converter 19. Both beam splitters 13 and 14, which are also known as dichroic filters, may be so-called beam splitter cubes, and are thus not identical since the beam splitter 14 is adapted to pass visible light through, which is incident on one side of it, and deflect the greenish light from the image converter incident on its other side. On the other hand, the beam splitter 13 is adapted to let through all visible light and only to deflect the invisible laser light. The light from the image converter 19 deflected in the image splitter 14 is focused together with the light rays from the beam splitter 13 towards a second focal plane 16 in the monocular telescope and is thus superimposed on the ordinary monocular telescope image. Since only the light rays coming from the laser light pass the image converter, it is avoided that the ordinary monocular telescope image is deteriorated although an image converter is utilized to generate a visible spot of invisible laser light. The image of the laser spot coming from the image converter will be somewhat greater than the imagae of the laser spot from the visible laser light in the means according to Figure 1. This is of subordinate importance however, since the central point of the spot can easily be distinguished even so. As a result of such as blows or shocks during transport, the image converter 19 or any of the units 13, 14, 17-21 may be given incorrect alignment, resulting in incorrect information as to the actual direction of the laser light source 10. In order that the means can be calibrated, a glass plate with clear marking, e.g. cross-hairs, is placed at the focal plane 11 of the monocular telescope objective. By illuminating the cross-hairs with light of approximately the same wave-length as that of the laser 10 and also with visible light two images of the cross-hairs are obtained at the second focal plane 16 in the monocular telescope. One image is obtained directly in the monocular telescope via the lenses and beam splitters 12-15, while the other image is obtained with the aid of the image converter 19. The means is adjusted by one of the units 13, 14, 17-21 being adjusted so that both images coincide. Since continous illumination is required in the calibration, a light source 22 giving continous light is used in this case, and not the laser 10 which only provides short light pulses. The light source 22 can convetionally be a light emitting diode, situated to one side of the focal plane 11. Part of a second embodiment of an alignment means in accordance with the invention is illustrated in Figures 3 and 4, Figure 3 being a plan of the means and Figure 4 a side-view from the right of a part of the means according to Figure 3. The laser light source and transmission optics are not depicted in the Figures. The members having direct counterpart in previous Figures have been provided with the same reference numerals as in these Figures. Members which have a principly similar task as the members in Figure 2 have been provided with reference numerals exceeding the value of the corresponding numerals in Figure 2 by 100. Only a single beam splitter is utilized in this means. The beam splitter comprises a beam splitter cube 30 having a beam splitting surface denoted by a diagonal line across the cube in Figure 3, and extending at right angles to the plane of the paper. The light rays in the monocular telescope are collimated by a convergent lens 112 and are incident on the beam splitter 30. The latter is adapted to let through visible light incident from the right in Figure 3, i.e. incident to the plane of the paper in Figure 4. The light is then incident on a convergent lens 115, which focuses it towards the eyepiece 6. The invisible light is deflected in the beam splitter 30 towards a convergent lens 117 and further towards a prism 31, which in turn reflects the light towards a prism 32. In Figure 3 the prism 32 is under the prism 31 and is therefore not visible in this Figure. The light is reflected in the prism 32 and is focused on the input surface of the image converter 19, which is hidden to a large extent in Figure 3. In this case as well, the image converter is also situated spaced from the monocular telescope axis 7, and is thus only passed through by light rays from the laser source. The visible light from the output of the image converter is reflected by two prisms 33 and 34 towards a collimater lens 121 and are then incident on the beam splitter 30. The latter is also adapted to deflect the greenish light coming from the lens 121, this light coming from the image converter 19, to the left in Figure 1, i.e. in the plane of the paper in Figure 4. The light is then incident on the lens 115 and is superimposed on the ordinary monocular telescope image. Other reflecting members than prisms can of course be used instead of the prisms 31-34. The means in accordance with this embodiment can also be adjusted with the aid of cross-hairs in the focal plane 11 in the same way as the means according to Figure 2. Both illustrated embodiments can naturally be changed within the scope of the claims. For example, the image converter can be used together with a monocular telescope with more than two focal planes. It is also conceivable to place the beam splitters in ray bundles which are not parallel.

Claims: 1. Alignment means for a light source (10) emitting invisible laser light, said means comprising: a monocular telescope (5,6); a reflecting prism (4) adapted for deflecting a part of the emitted laser light and reflecting it to the objective (5) of the monocular telescope, such that the reflected rays are at least practically parallel to the rays incident on the prism (4); an image converter (19) for generating a visible image of the reflected laser light, characterized in that the image converter (19) is situated spaced from the optical axis (7) of the monocular telescope (5,6) and in that the alignment means also includes members (13, 17, 18, 30, 117, 31, 32) for deflecting the reflected laser rays from the region around the optical axis of the monocular telescope to the input of the image converter (19), and means (20, 21, 14, 33, 34, 121, 30) for deflecting light rays from the output of the image converter (19) to the region round the optical axis (7) of the monocular telescope (5,6) such that the image of the laser rays now made visible by the image converter (19) are superimposed on the ordinary monocular telescope image. 2. Alignment means as claimed in claim 1, characterized in that said members for deflecting the reflected laser rays include a first beam splitter (13) and a first reflecting member (18), and in that the means for deflecting light rays from the output of the image converter (19) include a second reflecting member (20) and a second beam splitter (14). 3. Alignment means as claimed in claim 1, characterized in that said members for deflecting the reflected laser rays include a beam splitting cube (30) and a first (31) and a second (32) reflecting member, in that said means for deflecting light rays from the image converter include a third (33) and a fourth (34) reflecting member and said beam splitting cube (30), and in that the beam splitting cube (30), the beam converter (19) and said first, second, third and fourth reflecting members (31-34) are at least practically situated in a single plane, which at least practically is at right angles to the optical axis (7) of the monocular telescope (5,6). 4. Alignment means as claimed in claims 1 -3, characterized in that the monocular telescope includes a marking, e.g. cross-hairs, situated in a focal plane betwen the objective (5) and said members (13, 17, 18, 30, 117, 31, 32) for deflecting the reflected laser rays.

Inventors: HASSELSKOG, KARL JOHAN OLOV, SEVERINSSON, STEFAN ANDERS
Applicants: TELEFONAKTIEBOLAGET L M ERICSSON
Application year: 1988
Main classification: G02B23
IPC codes: G02B23