total correction of sun's altitude

简明释义

太阳高度总改正量

英英释义

例句

1.Sailors often rely on the total correction of sun's altitude for their celestial navigation.

水手们常常依赖于太阳高度的总修正进行天文导航。

2.The pilot adjusted the flight path based on the total correction of sun's altitude during the ascent.

在上升过程中，飞行员根据太阳高度的总修正调整了飞行路线。

3.The navigator calculated the total correction of sun's altitude to ensure accurate positioning at sea.

导航员计算了太阳高度的总修正以确保在海上的准确定位。

4.In astronomy, the total correction of sun's altitude is crucial for precise solar observations.

在天文学中，太阳高度的总修正对于精确的太阳观测至关重要。

5.When calculating the total correction of sun's altitude, factors like atmospheric refraction must be considered.

在计算太阳高度的总修正时，必须考虑大气折射等因素。

作文

The measurement of solar altitude is crucial in various fields, including astronomy, meteorology, and even in the design of solar panels. Understanding how to determine the sun's position in the sky can significantly improve our efficiency in utilizing solar energy. One essential concept related to this measurement is the total correction of sun's altitude, which refers to the adjustments made to account for various factors that affect the apparent position of the sun. Firstly, it is important to recognize that the sun does not follow a perfectly predictable path across the sky. Its altitude, or angle above the horizon, can be influenced by several variables, such as atmospheric refraction, the observer's geographical location, and the time of year. Atmospheric refraction occurs when sunlight passes through layers of the atmosphere with varying densities, bending the light and causing the sun to appear higher in the sky than it actually is. This effect is particularly noticeable when the sun is near the horizon, leading to discrepancies in altitude measurements.Moreover, the earth's tilt and its elliptical orbit around the sun also contribute to changes in solar altitude throughout the year. The total correction of sun's altitude involves calculating these variations to ensure accurate readings. For instance, during the summer solstice, the sun reaches its highest point in the sky, while during the winter solstice, it is at its lowest. Observers must take these seasonal changes into account when determining the sun's altitude at any given time.In addition to these natural factors, the observer's latitude plays a significant role in calculating solar altitude. Different locations on Earth experience varying angles of sunlight due to the curvature of the planet. For example, those living closer to the equator will have a more direct overhead sun during certain times of the year, while those at higher latitudes will experience a lower sun angle. Therefore, the total correction of sun's altitude must include adjustments based on the observer's specific location.Furthermore, technological advancements have allowed for more precise calculations of solar altitude. With the use of software and applications, individuals can now input their geographical coordinates and receive real-time data on the sun's position, including the necessary corrections. This has significant implications for solar energy systems, where maximizing sunlight exposure is essential for efficiency. By applying the total correction of sun's altitude, solar panel installations can be optimized for maximum energy capture, leading to greater sustainability efforts.In conclusion, the total correction of sun's altitude is a vital aspect of accurately measuring the sun's position in the sky. It encompasses various factors, including atmospheric refraction, seasonal changes, and the observer's geographical location. As we continue to harness solar energy and improve our understanding of the sun's behavior, mastering this concept will be essential for both scientific research and practical applications in renewable energy. By acknowledging and correcting for these variables, we can enhance our ability to utilize solar power effectively and responsibly.

太阳高度的测量在天文学、气象学甚至太阳能电池板设计等多个领域都至关重要。理解如何确定太阳在天空中的位置可以显著提高我们利用太阳能的效率。与此测量相关的一个基本概念是太阳高度的总修正，它指的是对影响太阳表观位置的各种因素进行的调整。首先，重要的是要认识到太阳并不沿着一个完全可预测的路径在天空中移动。太阳的高度或相对于地平线的角度可能会受到多种变量的影响，例如大气折射、观察者的地理位置和季节变化。大气折射发生在阳光穿过具有不同密度的气层时，光线弯曲，使得太阳看起来比实际位置更高。这种效应在太阳接近地平线时尤为明显，导致高度测量出现差异。此外，地球的倾斜和围绕太阳的椭圆轨道也会导致太阳高度在一年中的变化。太阳高度的总修正涉及计算这些变化，以确保读数的准确性。例如，在夏至期间，太阳在天空中的位置达到最高，而在冬至期间，则处于最低。观察者必须考虑这些季节性变化，以确定在任何给定时间太阳的高度。除了这些自然因素外，观察者的纬度在计算太阳高度时也起着重要作用。地球上的不同位置由于地球的曲率而经历不同的阳光角度。例如，生活在靠近赤道的人在某些时候会有更直接的阳光，而生活在高纬度地区的人则会经历较低的太阳角度。因此，太阳高度的总修正必须包括基于观察者特定位置的调整。此外，技术进步使得太阳高度的更精确计算成为可能。通过使用软件和应用程序，个人现在可以输入他们的地理坐标，并获得关于太阳位置的实时数据，包括必要的修正。这对太阳能系统具有重要意义，因为最大化阳光暴露对效率至关重要。通过应用太阳高度的总修正，太阳能电池板的安装可以优化以实现最大能量捕获，从而促进更大的可持续发展努力。总之，太阳高度的总修正是准确测量太阳在天空中位置的一个重要方面。它涵盖了各种因素，包括大气折射、季节变化和观察者的地理位置。随着我们继续利用太阳能并改善对太阳行为的理解，掌握这一概念对于科学研究和可再生能源的实际应用将至关重要。通过承认并纠正这些变量，我们可以增强有效和负责任地利用太阳能的能力。