Supporting Information for "Nine Martian Years of polar caps observations by SPICAM-IR"
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This dataset contains several additional figures and data for the "Nine Martian Years of polar caps observations by SPICAM-IR". Data and additional figures play special role in this publication, since we use a lot of different representations (seasonal, spatial and cap edges) of sparse dataset in our work. It also includes processed SPICAM-IR CO<sub>2</sub> ice equivalent width and water index for orbits without artifacts or distortions and with normal signal-to-noise ratio (>20).<br> <strong>Data Set S1 </strong><br> This Data Set (spicam_obs.csv) contains CO<sub>2</sub> ice equivalent width and water index for orbits without artifacts or distortions and with normal signal-to-noise ratio (>20) and all required observational geometry in a form of csv table. In this file there are 13 following columns: orbit: name of orbit as in PSA 1B files spec_num: number of spectrum in this file starting from zero lat: center latitude of field of view lon: center longitude of field of view ls: solar longitude of observation local_time: local time of observation incidence: incidence angle alt_spc: altitude of observation, which determines FOV size co2ice_index: equivalent width of CO ice 1.43 m band h2oice_index: index of 1.5 m water ice band albedo: albedo at 1.37 m, out of major absorption bands snr: signal-to-noise ratio measure around 1.37 m, out of major absorption bands martian_year: Martian Year Using this dataset one can plot all of the figures in the original paper, except for spectra. <strong>Data Set S2</strong><br> This Data Set (figure4.txt) contains data from Figure 4 in the original paper. Description of the figure:<br> Diversity of ice spectra on south pole. (Blue on picture): Slab ice in winter, Ls: 144.15, latitude: -58.7, longitude: 257.58, orbit: 10902A01, 1.43 µm band width: 30.5 nm; (Orange on picture): Bright CO2 ice, Ls: 253.08, latitude: -86.23, longitude: 315.70, orbit: 1943A01, 1.43 µm band width: 16.4 nm; (Green on picture): Cryptic region with almost no CO<sub>2</sub> ice, Ls: 213.12, latitude: -82.52, longitude: 122.06, orbit: 4169A01, 1.43 µm band width: 1.4 nm; (Red on picture): Water ice outside of cap in winter in the Hellas basin, Ls: 117.01, latitude: -42.97, longitude: 83.266, orbit: 20144A03, water ice index: 0.47; (Purple on picture): South permanent cap in the middle of summer, Ls: 322.85, latitude: -86.06, longitude: 311.33, orbit: 19015A01, 1.43 µm band width: 12.1 nm; (Brown on picture): Fine grained CO2 ice in the spring, Ls: 195.30, latitude: -64.90, longitude: 298.47, orbit: 8867A01, 1.43 µm band width: 6.6 nm <strong>Data Set S3</strong><br> This Data Set (figure5.txt) contains data from Figure 5 in the original paper. Description of the figure:<br> Diversity of ice spectra on north pole and spectrum of water ice clouds. (Blue on picture): Deep CO2 ice on North pole, Ls: 14.48, latitude: 85.72, longitude: 134.13, orbit: 5161A01, 1.43 µm band width: 20.6 nm; (Orange on picture): ”Cryptic”-like spectra in the end of winter, Ls: 332.38, latitude: 57.47, longitude: 82.96, orbit: 19074A01, 1.43 µm band width: 10.45 nm; (Green on picture): Spectrum with high water ice index on North pole, Ls: 107.88, latitude: 84.74, longitude: 34.69, orbit: 1002A01, water ice index: 0.758; (Red on picture): Water ice cloud in aphelion cloud belt, Ls: 114.94, latitude: 11.98, longitude: 254.08, orbit: 8336A01, water ice index: 0.146. <strong>Data Set S4</strong><br> This Data Set (figure6_bottom.txt, figure6_middle.txt, figure6_top.txt) contains data from Figure 6 in the original paper. Description of the figure:<br> Seasonal maps of CO<sub>2</sub> 1.43 µm equivalent width (top), water ice index (middle), and water ice index in log scale for the morning (bottom). <strong>Data Set S5</strong><br> This Data Set (figure9.txt) contains data from Figure 9 in the original paper. Description of the figure:<br> Outer crocus line for the south cap for all Martian Years combined. Orange points (on the figure) represent anti-cryptic part (from 260° to 60° east longitude) and cryptic part (from 60° to 260° east longitude). <strong>Data Set S6</strong><br> This Data Set (figure10.txt) contains data from Figure 10 in the original paper. Description of the figure:<br> Outer crocus line for the north cap for all Martian Years combined. Different colors (on the figure) represent different Martian Years.
本数据集为《SPICAM-IR观测火星极冠的九个火星年》一文补充了多组图表与数据。鉴于本文工作中针对稀疏数据集采用了多种不同的呈现方式(季节性、空间分布以及极冠边缘特征),补充数据与图表在该出版物中具有特殊意义。本数据集还包含经过预处理的SPICAM-IR二氧化碳(CO₂)冰等效宽度与水指数数据,对应轨道无伪影、无畸变且信噪比正常(>20)。 **数据集S1** 本数据集(spicam_obs.csv)以CSV表格形式存储了无伪影、无畸变且信噪比正常(>20)的轨道对应的CO₂冰等效宽度、水指数,以及所有必要的观测几何参数。该文件共包含13个字段: - orbit:对应行星科学档案(PSA)1B文件中的轨道名称 - spec_num:该文件中光谱的编号,从0开始计数 - lat:视场中心纬度 - lon:视场中心经度 - ls:观测时的太阳经度 - local_time:观测当地时间 - incidence:入射角 - alt_spc:决定视场大小的观测高度 - co2ice_index:1.43 μm波段CO₂冰的等效宽度 - h2oice_index:1.5 μm波段水冰的特征指数 - albedo:1.37 μm波段(避开主要吸收带)的反照率 - snr:1.37 μm波段(避开主要吸收带)的信噪比测量值 - martian_year:火星年 利用本数据集可复现原论文中除光谱图之外的全部图表。 **数据集S2** 本数据集(figure4.txt)包含原论文中图4的相关数据。该图表说明如下: 南极冰光谱的多样性。(图中蓝色曲线):冬季板状冰,太阳经度Ls=144.15,纬度=-58.7,经度=257.58,轨道编号10902A01,1.43 μm波段宽度=30.5 nm;(图中橙色曲线):明亮的CO₂冰,Ls=253.08,纬度=-86.23,经度=315.70,轨道编号1943A01,1.43 μm波段宽度=16.4 nm;(图中绿色曲线):几乎无CO₂冰的隐秘区,Ls=213.12,纬度=-82.52,经度=122.06,轨道编号4169A01,1.43 μm波段宽度=1.4 nm;(图中红色曲线):冬季赫拉斯盆地(Hellas)极冠外的水冰,Ls=117.01,纬度=-42.97,经度=83.266,轨道编号20144A03,水冰指数=0.47;(图中紫色曲线):盛夏时节的南极永久极冠,Ls=322.85,纬度=-86.06,经度=311.33,轨道编号19015A01,1.43 μm波段宽度=12.1 nm;(图中棕色曲线):春季细粒CO₂冰,Ls=195.30,纬度=-64.90,经度=298.47,轨道编号8867A01,1.43 μm波段宽度=6.6 nm **数据集S3** 本数据集(figure5.txt)包含原论文中图5的相关数据。该图表说明如下: 北极冰光谱多样性与水冰云光谱。(图中蓝色曲线):北极深层CO₂冰,Ls=14.48,纬度=85.72,经度=134.13,轨道编号5161A01,1.43 μm波段宽度=20.6 nm;(图中橙色曲线):冬末“隐秘区”类光谱,Ls=332.38,纬度=57.47,经度=82.96,轨道编号19074A01,1.43 μm波段宽度=10.45 nm;(图中绿色曲线):北极区域高水冰指数光谱,Ls=107.88,纬度=84.74,经度=34.69,轨道编号1002A01,水冰指数=0.758;(图中红色曲线):远日点云带中的水冰云,Ls=114.94,纬度=11.98,经度=254.08,轨道编号8336A01,水冰指数=0.146 **数据集S4** 本数据集(figure6_bottom.txt、figure6_middle.txt、figure6_top.txt)包含原论文中图6的相关数据。该图表说明如下: CO₂ 1.43 μm等效宽度的季节性分布图(上半部分)、水冰指数季节性分布图(中间部分),以及晨间水冰指数的对数坐标分布图(下半部分) **数据集S5** 本数据集(figure9.txt)包含原论文中图9的相关数据。该图表说明如下: 整合所有火星年的南极极冠外缘番红花边界线(crocus line)。图中橙色点代表反隐秘区(东经260°至60°)与隐秘区(东经60°至260°)。 **数据集S6** 本数据集(figure10.txt)包含原论文中图10的相关数据。该图表说明如下: 整合所有火星年的北极极冠外缘番红花边界线(crocus line)。图中不同颜色代表不同的火星年。



