一、基本信息
蔡玉珍,讲师,硕士生导师,主要研究方向为月球微波遥感和类地行星的地形粗糙度,旨在研究电磁波在行星表面的物理散射机制,并且分析地形起伏程度与地质活动的起源和演化的关联。至今共发表国际期刊论文多篇,参与国家自然科学基金面上项目,主持厅局级纵向课题一项。
二、教育经历
2012.09-2019.01,北京大学,摄影测量与遥感,博士
2007.09-2011.06,长安大学,测绘工程,学士
三、工作经历
2021.07-至今,新利luck在线·(中国)有限公司官网,讲师
2019.04-2021.06,中山大学,大气科学学院,博士后
三、主要科研项目
[1] 厅局级纵向课题,基于雷达探测仪数据对月球浅表层介电特性的研究,2022-2023,主持.
[2] 国家自然科学基金面上项目,月球极区雷达异常撞击坑特征与成因分析,2016-2019,参与.
四、近期主要论文
[1] Cai, Y. and Fa, W. (2020), Meter‐scale topographic roughness of the Moon: The effect of small impact craters, Journal of Geophysical Research: Planets, 125, e2020JE006429.
[2] Cai, Y. and Xiao, Z. Y., Ding, C. Y., and Cui, J. (2020), Fine debris flows formed by the Orientale Basin, Earth Planet. Phys., 4(3): 212-222.
[3] Ding C. Y., Cai, Y., Xiao, Z. Y., et al. (2020). A rocky hill on the continuous ejecta of Ziwei crater revealed by the Chang’e-3 mission. Earth Planet. Phys., 4(1), 1–6.
[4] Fa, W., Cai, Y. and Z. Xiao, and W. Tian (2016), Topographic roughness of the northern high latitudes of Mercury from MESSENGER Laser Altimeter data, Geophysical Research Letters, 43.
[5] Fa, W., and Cai, Y. (2013), Circular polarization ratio characteristics of impact craters from Mini-RF observations and implications for ice detection at the polar regions of the Moon, Journal of Geophysical Research: Planets, 118.
[6] Ding, C., Xiao, Z., Wu, B., Li, Y., Prieur, N. C., Cai, Y., et al. (2020). Fragments delivered by secondary craters at the Chang’e 4 landing site. Geophysical Research Letters, 47, e2020GL087361.
五、联系方式
地址:湖南省长沙市天心区万家丽南路二段960号工科二号楼B421
电子邮箱: yzcai@csust.edu.cn
热烈欢迎对行星科学感兴趣的同学联系报考!
一、基本信息
蔡玉珍,讲师,硕士生导师,主要研究方向为月球微波遥感和类地行星的地形粗糙度,旨在研究电磁波在行星表面的物理散射机制,并且分析地形起伏程度与地质活动的起源和演化的关联。至今共发表国际期刊论文多篇,参与国家自然科学基金面上项目,主持厅局级纵向课题一项。
二、教育经历
2012.09-2019.01,北京大学,摄影测量与遥感,博士
2007.09-2011.06,长安大学,测绘工程,学士
三、工作经历
2021.07-至今,新利luck在线·(中国)有限公司官网,讲师
2019.04-2021.06,中山大学,大气科学学院,博士后
三、主要科研项目
[1] 厅局级纵向课题,基于雷达探测仪数据对月球浅表层介电特性的研究,2022-2023,主持.
[2] 国家自然科学基金面上项目,月球极区雷达异常撞击坑特征与成因分析,2016-2019,参与.
四、近期主要论文
[1] Cai, Y. and Fa, W. (2020), Meter‐scale topographic roughness of the Moon: The effect of small impact craters, Journal of Geophysical Research: Planets, 125, e2020JE006429.
[2] Cai, Y. and Xiao, Z. Y., Ding, C. Y., and Cui, J. (2020), Fine debris flows formed by the Orientale Basin, Earth Planet. Phys., 4(3): 212-222.
[3] Ding C. Y., Cai, Y., Xiao, Z. Y., et al. (2020). A rocky hill on the continuous ejecta of Ziwei crater revealed by the Chang’e-3 mission. Earth Planet. Phys., 4(1), 1–6.
[4] Fa, W., Cai, Y. and Z. Xiao, and W. Tian (2016), Topographic roughness of the northern high latitudes of Mercury from MESSENGER Laser Altimeter data, Geophysical Research Letters, 43.
[5] Fa, W., and Cai, Y. (2013), Circular polarization ratio characteristics of impact craters from Mini-RF observations and implications for ice detection at the polar regions of the Moon, Journal of Geophysical Research: Planets, 118.
[6] Ding, C., Xiao, Z., Wu, B., Li, Y., Prieur, N. C., Cai, Y., et al. (2020). Fragments delivered by secondary craters at the Chang’e 4 landing site. Geophysical Research Letters, 47, e2020GL087361.
五、联系方式
地址:湖南省长沙市天心区万家丽南路二段960号工科二号楼B421
电子邮箱: yzcai@csust.edu.cn
热烈欢迎对行星科学感兴趣的同学联系报考!