一、基本信息
蔡玉珍,講師,碩士生導師,主要研究方向為月球微波遙感和類地行星的地形粗糙度,旨在研究電磁波在行星表面的物理散射機制,并且分析地形起伏程度與地質活動的起源和演化的關聯(lián)。至今共發(fā)表國際期刊論文多篇,參與國家自然科學基金面上項目,主持廳局級縱向課題一項。
二、教育經(jīng)歷
2012.09-2019.01,北京大學,攝影測量與遙感,博士
2007.09-2011.06,長安大學,測繪工程,學士
三、工作經(jīng)歷
2021.07-至今,長沙理工大學,講師
2019.04-2021.06,中山大學,大氣科學學院,博士后
三、主要科研項目
[1] 廳局級縱向課題,基于雷達探測儀數(shù)據(jù)對月球淺表層介電特性的研究,2022-2023,主持.
[2] 國家自然科學基金面上項目,月球極區(qū)雷達異常撞擊坑特征與成因分析,2016-2019,參與.
四、近期主要論文
[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、聯(lián)系方式
地址:湖南省長沙市天心區(qū)萬家麗南路二段960號工科二號樓B421
電子郵箱: yzcai@csust.edu.cn
熱烈歡迎對行星科學感興趣的同學聯(lián)系報考!
一、基本信息
蔡玉珍,講師,碩士生導師,主要研究方向為月球微波遙感和類地行星的地形粗糙度,旨在研究電磁波在行星表面的物理散射機制,并且分析地形起伏程度與地質活動的起源和演化的關聯(lián)。至今共發(fā)表國際期刊論文多篇,參與國家自然科學基金面上項目,主持廳局級縱向課題一項。
二、教育經(jīng)歷
2012.09-2019.01,北京大學,攝影測量與遙感,博士
2007.09-2011.06,長安大學,測繪工程,學士
三、工作經(jīng)歷
2021.07-至今,長沙理工大學,講師
2019.04-2021.06,中山大學,大氣科學學院,博士后
三、主要科研項目
[1] 廳局級縱向課題,基于雷達探測儀數(shù)據(jù)對月球淺表層介電特性的研究,2022-2023,主持.
[2] 國家自然科學基金面上項目,月球極區(qū)雷達異常撞擊坑特征與成因分析,2016-2019,參與.
四、近期主要論文
[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、聯(lián)系方式
地址:湖南省長沙市天心區(qū)萬家麗南路二段960號工科二號樓B421
電子郵箱: yzcai@csust.edu.cn
熱烈歡迎對行星科學感興趣的同學聯(lián)系報考!