aperture mirror

简明释义

孔镜

英英释义

例句

1.A larger aperture mirror typically results in brighter images.

更大的光圈镜通常会导致更明亮的图像。

2.In astrophotography, the size of the aperture mirror is crucial for gathering light.

在天文摄影中，光圈镜的大小对收集光线至关重要。

3.Adjusting the aperture mirror can enhance the clarity of the images captured.

调整光圈镜可以增强拍摄图像的清晰度。

4.The telescope's performance greatly improves with a high-quality aperture mirror.

高质量的光圈镜显著提高了望远镜的性能。

5.The aperture mirror in this telescope allows for better observation of distant galaxies.

这款望远镜中的光圈镜允许更好地观察遥远的星系。

作文

The concept of an aperture mirror is fundamental in the field of optics and astronomy. An aperture mirror refers to a type of mirror that is designed with a specific opening or 'aperture' that allows light to pass through it. This design is crucial for telescopes and other optical instruments, as it determines the amount of light that can enter the system, thereby influencing the quality and clarity of the images produced. In essence, the larger the aperture mirror, the more light it can collect, leading to better resolution and detail in observations.In astronomical observations, the size of the aperture mirror plays a significant role in determining the capabilities of a telescope. For instance, professional observatories often utilize telescopes equipped with large aperture mirrors to capture faint celestial objects that are millions of light-years away. These large mirrors are typically made from glass or other reflective materials that can withstand various environmental conditions while providing high-quality reflections.Moreover, the design of the aperture mirror is not only about size but also about shape. Most astronomical mirrors are parabolic, which helps to focus incoming light to a single point, enhancing the telescope's ability to produce clear images. The precision with which these mirrors are crafted is vital; even the slightest imperfection can lead to distortions in the observed image, making the study of distant galaxies or nebulae difficult.In addition to their use in telescopes, aperture mirrors are also found in various other optical devices, such as cameras and microscopes. In photography, for example, the aperture controls exposure and depth of field, allowing photographers to manipulate how much light enters the camera and how sharp or blurred the background appears. Understanding how aperture mirrors work can significantly enhance one’s skills in photography, as it enables better control over the final image.The advancement of technology has also led to innovations in the manufacturing of aperture mirrors. Modern techniques allow for the production of mirrors that are not only larger but also lighter and more durable. This is particularly important in space telescopes, where weight is a critical factor, and mirrors must endure the harsh conditions of space. The Hubble Space Telescope, for example, features a primary aperture mirror that is 2.4 meters in diameter, demonstrating the significant advancements in mirror technology that have taken place over the years.In conclusion, the aperture mirror is a pivotal element in the realm of optics, especially in astronomy. Its ability to collect and focus light determines the effectiveness of various optical instruments. As technology continues to evolve, we can expect to see further improvements in the design and functionality of aperture mirrors, which will undoubtedly enhance our understanding of the universe and improve our capabilities in both scientific research and photography. The study of aperture mirrors not only enriches our knowledge of optics but also opens up new possibilities for exploration and discovery in the vast expanse of space.

“光圈镜”这一概念在光学和天文学领域中是基础性的。“光圈镜”指的是一种设计有特定开口或“光圈”的镜子，允许光线通过。这种设计对于望远镜和其他光学仪器至关重要，因为它决定了可以进入系统的光量，从而影响生成图像的质量和清晰度。简而言之，“光圈镜”越大，它能收集的光线就越多，从而导致更好的分辨率和观察细节。在天文观察中，“光圈镜”的大小在决定望远镜的能力方面扮演着重要角色。例如，专业天文台通常使用配备大型“光圈镜”的望远镜来捕捉距离数百万光年的微弱天体。这些大型镜子通常由玻璃或其他反射材料制成，能够承受各种环境条件，同时提供高质量的反射。此外，“光圈镜”的设计不仅仅关乎尺寸，还涉及形状。大多数天文镜子是抛物线形的，这有助于将入射光聚焦到一个点上，从而增强望远镜产生清晰图像的能力。这些镜子的精确制造至关重要；即使是最轻微的缺陷也会导致观察图像的失真，使得对遥远星系或星云的研究变得困难。除了在望远镜中的应用外，“光圈镜”还出现在其他各种光学设备中，如相机和显微镜。在摄影中，例如，光圈控制曝光和景深，使摄影师能够操纵进入相机的光量以及背景的清晰或模糊程度。了解“光圈镜”的工作原理可以显著提升一个人在摄影方面的技能，因为这使得对最终图像的更好控制成为可能。技术的进步也促进了“光圈镜”制造的创新。现代技术使得生产不仅更大而且更轻、更耐用的镜子成为可能。这在太空望远镜中尤为重要，因为重量是一个关键因素，而镜子必须经受住太空的恶劣条件。例如，哈勃太空望远镜的主“光圈镜”直径为2.4米，展示了多年来镜子技术的重大进步。总之，“光圈镜”是光学领域，尤其是天文学中的关键元素。它收集和聚焦光的能力决定了各种光学仪器的有效性。随着技术的不断发展，我们可以期待在“光圈镜”的设计和功能上看到进一步的改进，这无疑将增强我们对宇宙的理解，并提高我们在科学研究和摄影方面的能力。“光圈镜”的研究不仅丰富了我们对光学的知识，还为探索和发现浩瀚太空开辟了新的可能性。