Data for: Modeled Small-scale Crack Orientations on Martian Surface Rocks caused by Differential Insolation-Mobilized Water

Data files for the submitted Icarus paper: "Modeled Small-scale Crack Orientations on Martian Surface Rocks caused by Differential Insolation-Mobilized Water". Data files contain the results of the combination of geometric and radiative transfer models. Data files are for a specific depth, width and length of V-shaped crack (as specified in the filename, where d is the depth, w is the width, and l is the length). These files are for those runs with no diurnal or seasonal restrictions. The files themselves are in the following format: planetary latitude (degrees) \t Solar longitude (degrees) \t crack offset clockwise from north (degrees) \t total energy received by the bottom third of the crack (J). Energy is calculated using the dimensions in meters so these values should be scaled according to the actual dimensions of the crack or can be used as a relative energy for different geometries and orientations (as in the paper).本数据集为投稿至《伊卡洛斯》（Icarus）期刊的论文配套数据文件，论文标题为《由日照差异驱动的水体迁移导致火星表面岩石小型模拟裂纹取向》（"Modeled Small-scale Crack Orientations on Martian Surface Rocks caused by Differential Insolation-Mobilized Water"）。数据文件包含几何模型与辐射传输模型（radiative transfer model）结合的运算结果。 本次数据针对特定深度、宽度与长度的V形裂纹生成，相关参数已在文件名中标注：其中d代表裂纹深度，w代表裂纹宽度，l代表裂纹长度。所有数据均为未设置昼夜或季节限制的模拟运行结果。 数据文件格式如下： 行星纬度（°） 太阳经度（°） 裂纹相对于正北方向的顺时针偏移角（°） 裂纹底部三分之一区域接收的总能量（J）。 能量计算采用米制尺寸单位，因此可根据实际裂纹尺寸对数值进行缩放，或如论文所述，将其作为不同几何形态与取向的相对能量参考值。