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    • 54. 发明授权
    • Cooled field optical system for infrared telescopes
    • 用于红外望远镜的冷却场光学系统
    • US4521068A
    • 1985-06-04
    • US484644
    • 1983-04-13
    • Joachim Schulte in den Baumen
    • Joachim Schulte in den Baumen
    • G01J5/06G02B5/00G02B17/06G02B23/02G02B23/16
    • G02B17/0663G01J5/061G02B17/061G02B23/02G02B23/16G02B5/005G02B17/0652
    • A cooled field optical system which serves for imaging the exit pupil of an infrared telescope with primary mirror having a central hole (Cassegrain system) onto a cooled annular diaphragm (9) which defines the field of view of the detector (14) used. It contains a field mirror (6) which is arranged behind the field diaphragm (5) of the telescope and whose focal length and distance from the field diaphragm are so selected that the image of the exit pupil is produced in the direct vicinity of the rear side of the field diaphragm (5) with a central vignetting which is greater than or equal to the aperture (15) of the field diaphragm (5). For deflection out of the coaxial ray path there is used an annular mirror (8) which is inclined to the optical axis and is arranged directly behind the field diaphragm (5). It has an elliptical hole the projected size of which is approximately the same as the size of the free passage (15) in the field diaphragm (5).
    • 一种冷却场光学系统,其用于对具有中心孔(卡塞格林系统)的主镜的红外望远镜的出射光成像到限定使用的检测器(14)的视场的冷却的环形隔膜(9)上。 它包括设置在望远镜的场隔膜(5)后面的场反射镜(6),并且其焦距和距离场光阑的距离被选择成使得出射光瞳的图像在后方直接附近产生 具有大于或等于场隔膜(5)的孔(15)的中心渐晕的场光阑(5)的一侧。 为了偏离同轴射线路径,使用与光轴倾斜并且直接设置在场隔膜(5)的后方的环形反射镜(8)。 它具有椭圆形孔,其投影尺寸与场隔膜(5)中的自由通道(15)的尺寸大致相同。
    • 55. 发明授权
    • Method and apparatus for aligning an optical system
    • 用于对准光学系统的方法和装置
    • US4471448A
    • 1984-09-11
    • US300073
    • 1981-09-08
    • Samuel G. L. Williams
    • Samuel G. L. Williams
    • G01B11/27G01J9/00G02B17/06G05B13/04G01N21/00
    • G02B17/0631G01B11/27G01J9/00G02B17/0663
    • A complex optical system may be aligned by means of a technique in which an analytical model of the system is utilized which is assumed to be capable of essentially optimal performance. A physical example of the same system design is then assembled and a plurality of performance characteristics measured. A plurality of specific adjustments are then calculated which would have the effect of degrading the performance of the analytical model to equal that measured for the physical example, whereupon compensating physical adjustments are made to the physical example. For many applications, the performance measurements may relate to aberrations to the wavefront of the point source image quantified by means of a Hartmann mask or the like. In that event, the estimation technique may be a straight-forward linear approximation technique including possible damping and/or weighting factors. The performance measurements may also be related to the intensity function associated with the image of a point source, in which case a second order estimation technique is required.
    • 复杂的光学系统可以通过使用系统的分析模型被利用的技术进行对准,该技术被认为能够基本上是最佳的性能。 然后组装相同系统设计的物理示例并测量多个性能特征。 然后计算多个具体的调整,其将具有将分析模型的性能降级到与物理实例所测量的性能相等的效果,由此补偿物理实例的物理调整。 对于许多应用,性能测量可以涉及通过Hartmann掩模等量化的点源图像的波前的像差。 在这种情况下,估计技术可以是包括可能的阻尼和/或加权因子的直线线性近似技术。 性能测量还可能与与点源的图像相关联的强度函数有关,在这种情况下需要二阶估计技术。
    • 58. 发明授权
    • Wide field reflective optical apparatus
    • 宽域反射光学装置
    • US3811749A
    • 1974-05-21
    • US29702872
    • 1972-10-12
    • HONEYWELL INC
    • ABEL I
    • G02B17/06G02B23/00G02B17/00
    • G02B23/06G02B17/0615G02B17/0642G02B17/0663
    • The disclosure describes a wide field reflective optical system comprising an afocal fore telescope and an imaging system. The afocal telescope comprises first and second confocal paraboloidal reflectors, an aperture stop located in front of the first reflector at a distance equal to its focal length, and a field stop located at the common focal point of the reflectors. The imaging system is an improvement of the Schmidt principle and comprises an aspheric corrector reflector that reflects radiation from the second paraboloidal reflector onto a plane reflector. The plane reflector is located in front of a spherical reflector that focuses radiation at its focal plane through an aperture in the plane reflector.
    • 本公开描述了一种包括无焦前望远镜和成像系统的宽场反射光学系统。 无焦点望远镜包括第一和第二共聚焦抛物面反射器,位于第一反射器前面的距离等于其焦距的孔径光阑,以及位于反射器的公共焦点处的场停止。 成像系统是Schmidt原理的改进,并且包括将来自第二抛物面反射器的辐射反射到平面反射器上的非球面校正器反射器。 平面反射器位于球面反射器的前面,其将辐射在其焦平面处通过平面反射器中的孔聚焦。