Dataset of "Large water inventory in a highly adsorptive regolith near the equator simulated by a Mars global climate model"

This dataset can be used for drawing all figures in the paper "Large water inventory in a highly adsorptive regolith near the equator simulated by a Mars global climate model" by M. Kobayashi, A. Kamada, T. Kuroda, H. Kurokawa, S. Aoki, H. Nakagawa, N. Terada. The following files are included: run1.zip, run2.zip, run3.zip, run4.zip, and run5.zip. Each zip file with a name beginning with "data" contains ascii files of Adsorption coefficient in kg/m3 (ads0.asc), Atmospheric water vapor column in kg/m2 (colwv2.asc), Effective diffusion coefficient in m2/s (dif2.asc), Porosity for the ice-free regolith (phi0.asc), Surface pressure in hPa (Ps.asc), Grain size in m (rd.asc), Pore size in m (rp.asc), Surface temperature in K (Ts.asc), Ground temperature in K (Tg.asc), Adsorbed water mass in kg/m3 (wga2.asc), Column adsorbed water mass in kg/m2 (wga2c.asc), Pore ice mass in kg/m3 (wgi2.asc), Column pore ice mass in kg/m2 (wgi2c.asc), Water vapor mass in the regolith in kg/m3 (wgv2.asc), and Column water vapor mass in the regolith in kg/m2 (wgv2c.asc). Data for numbers 1–8 have a horizontal resolution of T10 (corresponding to a triangular truncation at wavenumber 10) and a vertical layer (at the surface). Data for numbers 9–15 have a horizontal resolution of T10 and 17 ground layers down to 20 m. Each data starts from Ls=0° in the last year after 500 Martian years of calculations and is output in 3 Martian-day time intervals. The data files wga2c.asc and wgi2c.asc contain the layer values multiplied by the layer thicknesses added together from the surface. The data file wgv2c.asc contains the layer values multiplied by the layer thicknesses and the porosity added together from the surface. The zip file "run5.zip" only has the following data with a short time interval: Atmospheric water vapor column in kg/m2 (colwv2-s.asc) and Surface temperature in K (Ts-s.asc). These files have a horizontal resolution of T10 and a vertical layer (at the surface). Each data starts from Ls=0°, 0:00 at longitude 0° in the last year after 500 Martian years of calculations and is output in 1 hour time intervals.本数据集可用于复现M. Kobayashi、A. Kamada、T. Kuroda、H. Kurokawa、S. Aoki、H. Nakagawa、N. Terada所撰写的论文《基于火星全球气候模型模拟的赤道附近高吸附性风化层中的大量水储量》（"Large water inventory in a highly adsorptive regolith near the equator simulated by a Mars global climate model"）中的全部插图。 本数据集包含以下压缩文件：run1.zip、run2.zip、run3.zip、run4.zip以及run5.zip。 每个以"data"开头的压缩包内均包含如下ASCII格式文件： - 单位为kg/m³的吸附系数（ads0.asc） - 单位为kg/m²的大气水汽柱含量（colwv2.asc） - 单位为m²/s的有效扩散系数（dif2.asc） - 无冰风化层孔隙度（phi0.asc） - 单位为hPa的地表气压（Ps.asc） - 单位为m的粒径（rd.asc） - 单位为m的孔隙尺寸（rp.asc） - 单位为K的地表温度（Ts.asc） - 单位为K的地下温度（Tg.asc） - 单位为kg/m³的吸附水质量（wga2.asc） - 单位为kg/m²的柱吸附水质量（wga2c.asc） - 单位为kg/m³的孔隙冰质量（wgi2.asc） - 单位为kg/m²的柱孔隙冰质量（wgi2c.asc） - 单位为kg/m³的风化层内水汽质量（wgv2.asc） - 单位为kg/m²的风化层内柱水汽质量（wgv2c.asc） 其中编号1至8的数据的水平分辨率为T10（对应波数10的三角截断），垂直方向仅包含地表一层。编号9至15的数据的水平分辨率为T10，垂直方向包含17层地下土层，最大深度达20米。 所有数据均起始于500个火星年模拟结束后的最后一个火星年的太阳经度（Ls）0°处，并以3个火星日为时间间隔进行输出。其中wga2c.asc与wgi2c.asc文件存储的是各层数值乘以对应层厚度后，从地表至该层的累加总量。wgv2c.asc文件存储的是各层数值乘以对应层厚度与孔隙度后，从地表至该层的累加总量。 压缩包run5.zip仅包含以下高时间分辨率的数据： - 单位为kg/m²的大气水汽柱含量（colwv2-s.asc） - 单位为K的地表温度（Ts-s.asc） 上述文件的水平分辨率为T10，垂直方向仅包含地表一层。所有数据起始于500个火星年模拟结束后的最后一个火星年的经度0°处的Ls=0° 0:00时刻，并以1小时为时间间隔进行输出。