The present invention relates to a far-optical device, in particular a telescope or aiming telescope, comprising a reversal system and an adjustable optical magnification means with more than fourfold magnification.
If an object at a great distance is viewed with the naked eye it appears at a small angle. The purpose of any far-optical device is to magnify that small angle. The far-optical device thereform provides that an appearance angle which is as large as possible can pass into the eye of the viewer. At the same time it should be possible to overlook a piece of territory which is as large as possible.
In the case of zoomable far-optical devices of the general kind set forth, involving an adjustable magnification, it is particularly critical to be able to overlook a piece of territory which is as large as possible, over the entire magnification range.
The object of the invention is to improve far-optical devices of the general kind set forth, in that respect.
In accordance with the invention that is achieved in that the far-optical device has an optical beam deflection means which at all magnifications ensures a subjective field of view of the far-optical device of at least 22°, preferably between 22° and 24°, at least for light of a wavelength of about 550 nm.
By means of the optical beam deflection means, it is now possible to afford a subjective field of view of at least 22°, even at low levels of magnification, in particular at the lowest magnification, of the far-optical device. That was possible hitherto only at relatively high levels of magnification of far-optical devices of the general kind set forth. Accordingly, even at low levels of magnification, by means of the far-optical device according to the invention, the viewing person sees a larger piece of territory than the state of the art hitherto permitted.
In accordance with a further aspect of the invention the specified object is also attained if it is provided that the beam deflection means at the maximum magnification ensures a total focal length of the reversal system of between 11 mm and 7 mm, preferably between 10 mm and 8 mm.
Further details and features of the invention are explained with reference to the Figures described hereinafter, in which:
Two optical elements 3a and 3b are provided for magnifying the image and making it upright. In general these involve achromatic elements which for controlling chromatic aberration are desirably in the form of what are referred to as cemented lenses, that is to say lens arrangements which are bonded together. In the state of the art as also in the case of reversal systems or far-optical devices in accordance with the invention they appropriately have refractive powers of +20 dpt (dioptres) up to +53 dpt, preferably from +21 dpt to +35 dpt, particularly preferably in the range between +23 dpt and +26 dpt. In order to make the magnification of the illustrated aiming telescope adjustable, the optical elements 3a and 3b are movable along control grooves. Displacement of the optical elements 3a and 3b means that the intermediate image produced by the objective 4 in the objective-side image plane 9 is produced, with the changing imaging scale and in an upright position, in the eyepiece-side image plane 10. In the illustrated embodiment the spacing of the two image planes 9 and 10 is not changed by the displacement of the optical elements 3a and 3b. In the state of the art moreover it was also known additionally also to provide a field lens 11. That helps to pass the beam of rays, coming from the objective 4, of an object point at the edge of the field of view, through the narrow passage of the central tube 6 and the reversal system 1 respectively.
The change in the imaging scale by movement of the optical elements 3a and 3b along control grooves (not further shown in detail here) is known in the state of the art.
In order now to be able to ensure a subjective field of view of at least 22° in a far-optical device with a maximum magnification or a maximum zoom of greater than four times, even at low levels of magnification, the invention provides an optical beam deflection means 2. That is shown in an embodiment in
The optical beam deflection means 2 however can equally well be arranged in the form of a separate component, separately from the reversal system 1, in the far-optical device. On the other hand however it is also possible for the optical beam deflection means 2 according to the invention to be embodied by a suitable configuration of the lenses 11, 3a and 3b. It is desirably provided that the optical beam deflection means ensures the subjective field of view of at least 22°, preferably between 22° and 24°, in relation to an optical magnification means, preferably of the reversal system, with an at least fivefold and preferably at an at least sixfold, maximum magnification, at all magnification stages. For better control of chromatic aberration it has been found to be appropriate for the optical beam deflection means 2 to have preferably two lenses 7 which are bonded together, that is to say cemented lenses. It would however also be conceivable for the optical beam deflection means 2 to be in the form of an individual lens.
It has proven to be desirable for the optical beam deflection means 2 to be arranged on the side of the reversal system 1, which faces towards the eyepiece 5. In that respect positioning on the side of the eyepiece-side image plane 10, which faces away from the eyepiece 5, is advantageous.
A solution which is structurally particularly simple provides that the optical beam deflection means 2 is arranged fixedly, that is to say not movably with respect to the central tube 6. In certain embodiments however it has also proven to be necessary for the optical beam deflection means 2 to be designed to be movable, that is to say generally displaceable along the optical axis.
Hitherto, in current aiming telescopes, the central tube is of an outside diameter of between 30 mm and 35 mm. That is naturally reckoned without any adjusting towers 8 or the like which may be present. That dimension for the central tube 6 is desirably also retained in the case of aiming telescopes according to the invention.
In general it is desirable for the optical beam deflection means 2 to have a refractive power of between −20 dpt (dioptres) and −40 dpt, preferably between −27 dpt and −37 dpt. In a specific example, the refractive power provided is −27.03 dpt, in which case a subjective field of view of 23.5° is achieved at all levels of magnification.
The size of the subjective field of view 2 ω′ is determined by means of angle measurement. The corresponding measurement structure for testpieces with a real exit pupil is shown in
Measurement of the total focal length of a reversal system is effected in accordance with DIN 58189 (issued in May 1996) and can be carried out with commercially available testing apparatuses.
Number | Date | Country | Kind |
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A 1220/2005 | Jul 2005 | AT | national |
The present application is a continuation of U.S. patent application Ser. No. 15/350,397, filed on Nov. 14, 2016, which is a continuation of U.S. patent application Ser. No. 14/305,849, filed on Jun. 16, 2014, issued as U.S. Pat. No. 9,529,185, which is a continuation of U.S. patent application Ser. No. 13/234,705, filed on Sep. 16, 2011, issued as U.S. Pat. No. 8,786,947, which is a continuation of U.S. patent application Ser. No. 12/793,073, filed on Jun. 3, 2010, issued as U.S. Pat. No. 8,054,544, which is a continuation of U.S. patent application Ser. No. 11/453,983, filed on Jun. 16, 2006, issued as U.S. Pat. No. 7,742,228, which claims priority from Austrian Patent Application No. A1220/2005, filed on Jul. 20, 2005, the disclosures of which are hereby incorporated herein by reference.
Number | Date | Country | |
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Parent | 15350397 | Nov 2016 | US |
Child | 16797558 | US | |
Parent | 14305849 | Jun 2014 | US |
Child | 15350397 | US | |
Parent | 13234705 | Sep 2011 | US |
Child | 14305849 | US | |
Parent | 12793073 | Jun 2010 | US |
Child | 13234705 | US | |
Parent | 11453983 | Jun 2006 | US |
Child | 12793073 | US |