搜索资源列表
Projection_Gauss
- 用于测量与地图制图的高斯投影转换，提供了北京54、全国80、WGS84三个坐标系下的正算、反算。输出结果精确到小数点后7位。-for measuring and mapping the Gauss projection conversion, the Beijing 54, 80, 3 WGS84 coordinates the count is, anti-counting. Output accurate to seven decimal places.
GaussProject
- 大地测量高斯投影坐标计算。可以正算，也可以反算。
BASIC-positonconvert
- 用BASIC语言实现54坐标系参数下的的正反算。对于84坐标系，反算时的底点纬度可以用直接法算-BASIC language with 54 coordinate system parameters to achieve the balance of positive and negative. Coordinate system for the 84. Anti-count at the end point of latitude at the time of the direct metho
Gauss
- 高斯投影正算反算功能，实现高斯投影的正算和反算功能-The Gauss calculte descr iption
fansuan
- 大地测量中的高斯坐标反算，以前写的小程序-Geodetic coordinates in the inverse Gaussian, used to write small programs
gauuss
- 关于高斯投影的正算和反算，里面含有四种大地基准，方便进行各类运算-Positive operator on the Gaussian projection and the inverse, which contains four geodetic datum, to facilitate operation
satellite-second
- 卫星的轨道反算，程序用MFC编写，界面美观大方，适用于初学者-Anti-satellite orbit calculation, the program written with MFC, beautiful interface, suitable for beginners
xyz2neu
- XYZ坐标转为GLOBK或者QOCA中的NEU，以及大地测量中大地线反解问题，即由经纬度解算大地线长度-convert XYZ coordinates into NEU in GLOBK or NEU, and geodetic earth line inverse solution, that solution by the latitude and longitude Geodetic Line length
Ephemeris_And_Orbital
- 利用卫星的星历参数计算其轨道，同时还能根据速度和加速度反算星历参数，是基于MFC对话框的编程-Using satellite ephemeris parameters to calculate its orbit, while depending on the speed and acceleration of the inverse ephemeris parameters is based on MFC dialog programming
CL
- 自己做的几个涉及到测量的子程序，有坐标反算、排序、角度转换、时间处理、四舍六入、三维显示-Yourself a few involves measurement subroutine, are calculated by coordinates, sorting, Angle conversion, time processing, and six into four, three dimensional display and so on
ProjectionTransform
- 高斯正算，高斯反算，换带计算，用户坐标转GPS坐标-Gauss positive operators, inverse Gaussian, for band calculations, the user coordinate turn GPS coordinates
bessel
- 使用白塞尔方法进行大地主题解算，正算由大地线和大地方位角计算经纬度，反算有经纬度计算大地线长度和大地方位角(Using the white Searl method to solve the geodetic problem, we calculate the longitude and latitude by the geodesic and the earth azimuth, and calculate the geodesic length and the large local ang