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    • 4. 发明申请
    • ANTENNAS FOR SMALL SATELLITES
    • 天线小卫星
    • US20150162656A1
    • 2015-06-11
    • US14407396
    • 2013-06-11
    • UNIVERSITY OF FLORIDA RESEARCH FOUNDATION, INC.
    • Norman G. Fitz-CoyVivek ShirvanteShawn JohnsonKathryn Cason
    • H01Q1/28B64G1/44B64G1/10B64G1/22
    • H01Q1/288B64G1/105B64G1/222B64G1/443B64G1/66H01Q9/30H01Q19/106
    • Various embodiments of the present invention include assemblies and methods for utilizing antennas with high gain in small satellites. In one embodiment, a satellite comprising a payload configured for transmitting data is provided. The payload may include various components of the satellite, such as the attitude control system, electrical power system, and/or communication system. The satellite may be configured to communicate with one or more ground stations. The satellite includes a support structure comprising at least one deployable panel, wherein the support structure houses the payload. The satellite also includes at least one antenna coupled to the support structure, wherein the deployable panel is configured to cover the antenna in a non-deployed state and to expose the antenna in a deployed state.
    • 本发明的各种实施例包括在小型卫星中利用具有高增益的天线的组件和方法。 在一个实施例中,提供了包括被配置为用于发送数据的有效载荷的卫星。 有效载荷可以包括卫星的各种部件,例如姿态控制系统,电力系统和/或通信系统。 卫星可以被配置为与一个或多个地面站通信。 卫星包括支撑结构,该支撑结构包括至少一个可展开的面板,其中支撑结构容纳有效载荷。 所述卫星还包括耦合到所述支撑结构的至少一个天线,其中所述可展开面板被配置为以非展开状态覆盖所述天线并且在展开状态下露出所述天线。
    • 6. 发明授权
    • Telescope multiple discrete segment primary mirror
    • 望远镜多个离散段主镜
    • US07837340B2
    • 2010-11-23
    • US11782534
    • 2007-07-24
    • George Watters
    • George Watters
    • G02B5/08
    • G02B7/183B64G1/105G02B17/002G02B17/0694G02B23/16G02B27/0018
    • A method and apparatus is configured for reflecting a beam of light incident at a primary mirror by rotating a first mirror segment to align a selected facet of the mirror segment to be generally orthogonal to the principal axis. The first mirror segment is translated in a motion parallel to the principal axis to a first position such that the mirrored segment at a facet comprising a mirror is brought into alignment with at least one second mirrored segment to form at a facet a first parabolic mirror. The incident beam of light is then reflected by collimating the first parabolic mirror by rotation and translation of the first mirror segment to strike a first secondary element.
    • 一种方法和装置被配置为通过旋转第一反射镜部分来反射入射在初级反射镜上的光束,以将反射镜分段的所选择的小平面与主轴垂直。 第一镜片段以平行于主轴的运动平移到第一位置,使得包括镜的小面处的镜像片段与至少一个第二镜像片段对准,以在小平面处形成第一抛物面镜。 然后通过使第一反射镜段的旋转和平移来对第一抛物面反射镜进行准直以撞击第一次要元件来反射入射光束。
    • 7. 发明申请
    • TELESCOPE MULTIPLE DISCRETE SEGMENT PRIMARY MIRROR
    • 电话多重分段主要镜像
    • US20090027789A1
    • 2009-01-29
    • US11782534
    • 2007-07-24
    • George Watters
    • George Watters
    • G02B5/08
    • G02B7/183B64G1/105G02B17/002G02B17/0694G02B23/16G02B27/0018
    • A method and apparatus is configured for reflecting a beam of light incident at a primary mirror by rotating a first mirror segment to align a selected facet of the mirror segment to be generally orthogonal to the principal axis. The first mirror segment is translated in a motion parallel to the principal axis to a first position such that the mirrored segment at a facet comprising a mirror is brought into alignment with at least one second mirrored segment to form at a facet a first parabolic mirror. The incident beam of light is then reflected by collimating the first parabolic mirror by rotation and translation of the first mirror segment to strike a first secondary element.
    • 一种方法和装置被配置为通过旋转第一反射镜部分来反射入射在初级反射镜上的光束,以将反射镜分段的所选择的小平面与主轴垂直。 第一镜片段以平行于主轴的运动平移到第一位置,使得包括镜的小面处的镜像片段与至少一个第二镜像片段对准,以在小平面处形成第一抛物面镜。 然后通过使第一反射镜段的旋转和平移来对第一抛物面反射镜进行准直以撞击第一次要元件来反射入射光束。
    • 10. 发明授权
    • Spacecraft inertial attitude and rate sensor control system
    • US6158694A
    • 2000-12-12
    • US170986
    • 1998-10-13
    • Sankaran Gowrinathan
    • Sankaran Gowrinathan
    • B64G1/10B64G1/36B64G1/66
    • B64G1/361B64G1/363B64G1/66B64G1/105B64G2001/1057
    • Disclosed is a method and apparatus (1'; 1") for tracking a stellar body (22) using a telescope (9; 32) of a spacecraft (e.g., a satellite) (10; 10"). In accordance with an embodiment of the invention, the telescope (9; 32) is provided with gimbal supports (18a; 18b), and is maneuverable relative to the spacecraft (10; 10'). The stellar body (22) is acquired by the telescope (9; 32) so that the stellar body (22) is within the field of view (FOV) of the telescope (9; 32). After the stellar body (22) is acquired, an operation is performed for controlling the attitude of the spacecraft (10; 10') to within pre-established deadband limits, and, as a result, the spacecraft (10; 10') and telescope (9; 32) are each assumed to have a desired orientation relative to the stellar body (22). The stellar body tracking method of the invention is performed so as to maintain the telescope (9; 32) in an orientation wherein the stellar body (22) is within the field of view (FOV) of the telescope (9; 32), even if it occurs that one or more environmental disturbance forces impinge on the spacecraft (10; 10') and cause an undesired variation in the orientation of the spacecraft (10; 10') relative to the stellar body (22). The stellar body tracking method of the invention controllably points a pointing direction (line of sight) of the stellar body tracking system (1'; 1") independently of the spacecraft (10; 10'), for tracking the stellar body (22). In accordance with an aspect of this invention, spacecraft inertial position and rate information is derived for use in controlling the attitude of the spacecraft (10; 10'). In accordance with an embodiment of the invention, the pointing direction of the telescope (9; 32) is controllably pointed by maneuvering at least one of the telescope (9; 32) and a mirror (13") of the telescope (9; 32).