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本代码中的PDF文档和名为seclipse.m的matlab脚本可以用来预测当地日食的情况。
PDF document and a MATLAB script named seclipse.m that can be used to predict local circumstances of solar eclipses.
该计算机程序提供了太阳和月球在半影接触开始和结束时的时间和地心坐标,以及日食最大时的时间和坐标。
This computer program provides the universal times and topocentric coordinates of the Sun and Moon at the beginning and end of the penumbra contacts, and the time and coordinates at maximum eclipse.
此例程的源星历表为JPL二进制星历文件。
The source ephemeris for this routine is a JPL binary ephemeris file.
该应用程序使用了几个从Fortran版本的NOVA(海军天文台矢量天体测量子程序)源代码移植到MATLAB的函数,该源代码由美国海军天文台开发。
This application uses several functions ported to MATLAB from the Fortran version of the NOVAS (Naval Observatory Vector Astrometry Subroutines) source code developed at the United States Naval Observatory (www.usno.navy.mil/USNO/astronomical-applications/software-products/novas).
可从以下网址下载与Windows兼容的JPL二进制星历表文件。
JPL binary ephemeris files for Windows compatible computers can be downloaded at http://celestialandorbitalmechanicswebsite.yolasite.com/.
完整源码下载地址:
http://page2.dfpan.com/fs/9l0cfj22f2416289163/
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