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Verification of the Astronomical Almanac's algorithm for approximate the position of the sun

机译:验证天文学年历算法以近似太阳的位置

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With the consumption of the resources, it's important to develop clean solar energy that can solve the problem of energy shortage. Obtaining an accurate position of the sun is the premise of using the solar energy efficiently. An accurate solar position includes two factors that are elevation and azimuth. In the paper, Joseph J. Michalsky's algorithm for calculation of the solar position is verified that is taken from the American Astronomical Almanac. The algorithm has been written into program by Joseph J. Michalsky in FORTRAN. In the paper, it's has been adapted to visual C++ that can calculate the solar elevation and azimuth and errors or some places that less accurate are corrected. The Chinese Astronomical Almanac for the year 1985 doesn't tabulate elevation and azimuth. The quantities needed to calculate elevation and azimuth are the right ascension, the declination and the Greenwich mean sidereal time that are tabulated in the Almanac. Comparing those variables that calculated from the algorithm with the data from the Chinese Astronomical Almanac for the year 1985, it can be found that the biggest difference of the two ways is only 0.01 ° , 0.01 ° and O.OOOlh respectively, which prove the accuracy of the algorithm indirectly. The measured data that only include elevation comes from Basic Data of Geography in China written by Institute of Geography, Chinese Academy of Sciences. Comparing elevation given by the algorithm with the measured data, it shows that the algorithm can be accurate calculating the position of the sun in some extent. And the paper shows in detail the conversion from the local real solar time to Universal Time because the time in Basic Data of Geography in China is the local real solar time. Finally we notice that the 0.01° accuracy mentioned by other paper is not the accuracy of the elevation and azimuth of the sun, but the accuracy of the right ascension and declination. It's easy to understand why the difference of the results calculated by the algorithm and measured data is greater than 0.01 ° .
机译:随着资源的消耗,开发能够解决能源短缺问题的清洁太阳能非常重要。获得太阳的准确位置是有效利用太阳能的前提。准确的太阳位置包括两个因素,即海拔和方位角。在本文中,验证了约瑟夫·米哈尔斯基(Joseph J. Michalsky)用于计算太阳位置的算法,该算法取自《美国天文学年鉴》。该算法已由FORTRAN中的Joseph J. Michalsky写入程序中。在本文中,它已针对Visual C ++进行了修改,可以计算太阳高度和方位角以及错误或某些精度较差的地方已得到纠正。 1985年的中国天文年历没有列出海拔和方位角。计算高程和方位角所需的数量是在年历中列出的右上角,偏角和格林威治平均卫星实时时间。将这些算法计算出的变量与1985年中国天文历书的数据进行比较,可以发现两种方法的最大差异分别仅为0.01°,0.01°和0.001h,证明了准确性。间接算法。仅包含海拔的测量数据来自中国科学院地理研究所编写的《中国基本地理数据》。将算法给出的仰角与实测数据进行比较,表明该算法在一定程度上可以准确计算出太阳的位置。由于中国《地理基本数据》中的时间就是当地的实际太阳时间,因此本文详细地说明了从当地的实际太阳时间到世界时间的转换。最后,我们注意到其他论文提到的0.01°精度不是太阳的仰角和方位角的精度,而是右上角和偏角的精度。很容易理解为什么算法计算的结果与实测数据之差大于0.01°。

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