Reflectance spectra of orthoenstatite, clinoenstatite, and Peña Blanca Spring for "Reflectance spectra of synthetic Fe-free ortho- and clinoenstatites in the UV/VIS/IR and implications for remote sensing detection of Fe-free pyroxenes on planetary surfaces"

This data is supplementary to Markus et al. (2018) Reflectance spectra of synthetic Fe-free ortho- and clinoenstatites in the UV/VIS/IR and implications for remote sensing detection of Fe-free pyroxenes on planetary surfaces. Planetary and Space Science 159, 43–55. https://doi.org/10.1016/j.pss.2018.04.006 The dataset comprises reflectance spectra of orthoenstatite, clinoenstatite, the aubrite Peña Blanca Spring, and an additionally ground subsample of the orthoenstatite from ~0.25 to 17 µm as presented in Markus at al. (2018). First column gives wavelength in µm, second column gives reflectance. Incidence angle and emergence angles are both 15° with a resulting phase angle of 30°. If you use these spectra, please also cite the PSS publication.本数据集为Markus等人（2018年）研究成果的补充数据，原文题为《紫外/可见光/红外（UV/VIS/IR）波段下合成无铁斜方顽火辉石（orthoenstatite）与单斜顽火辉石（clinoenstatite）的反射光谱及行星表面无铁辉石（pyroxenes）遥感探测的启示》，发表于《行星与空间科学》第159卷，第43-55页，DOI: 10.1016/j.pss.2018.04.006。 本数据集包含Markus等人（2018年）研究中提及的斜方顽火辉石（orthoenstatite）、单斜顽火辉石（clinoenstatite）、Peña Blanca Spring顽火辉石无球粒陨石（aubrite），以及波段范围约0.25至17 μm的斜方顽火辉石研磨子样品的反射光谱。 数据第一列为以微米（μm）为单位的波长，第二列为反射率。实验中入射角与出射角均为15°，对应的相位角为30°。 若使用本光谱数据，请同时引用该《行星与空间科学》（PSS）期刊发表的论文。