人员
人员

位置: 首页 > 人员 > 专任教师 > 天文学系 > 正文

马任意

个人主页:

研究领域 黑洞吸积盘理论;高能辐射过程;宇宙学激波与高能宇宙射线

教育和工作经历
2001~2006 华中科技大学 博士
2006~2008 中科院上海天文台 博士后
2008~2010 韩国国立忠南大学 博士后
代表性文章或专著
1. Gong, X. L., Li, L. X., & Ma, R. Y. "A Disc-Corona Model for a Rotating Black Hole", Monthly Notices of the Royal Astronomical Society (Accepted)
2. Ma, R. Y., Ryu, D., & Kang, H. "Cosmic Rays Accelerated at Cosmological Shock Waves", J. Astrophys. Astr., 32, 301 (2011)
3. Edmon. P. P., Kang, H., Jones, T., & Ma, R. Y. "Non-thermal radiation from Type Ia supernova remnants", Monthly Notices of the Royal Astronomical Society, 414, 3521 (2011)
4. Yuan, F., Ma, R. Y., & Narayan, R. "A Simplified Global Solution for an Advection-dominated Accretion Flow", Astrophys. J., 679, 984 (2008)
5. Ma, R. Y., Yuan, F., & Wang, D. X. "Influence of the Magnetic Coupling Process on the Advection Dominated Accretion Flows around Black Holes", Astrophys. J., 671, 1981 (2007)
6. Ye, Y. C., Wang, D. X., & Ma, R. Y. "Magnetic coupling of a rotating black hole with advection-dominated accretion flows", New Astron., 12, 471 (2007)
7. Ma, R. Y., Wang, D. X., & Zuo, X. Q. "Influences of the magnetic coupling process on the spectrum of a disk covered by the corona", Astron. and Astrop., 453, 1 (2006)
8. Lei, W. H., Wang, D. X., & Ma, R. Y. "A Toy Model for Gamma-Ray Bursts in Type Ib/c Supernovae", Astrophys. J., 619, 420 (2005)
科研基金及项目
“Blazar伽玛辐射起源的重子模型”,国家自然科学基金主任基金项目
“Blazar的高能辐射机制及应用”,福建省自然科学基金面上项目
任教课程
大学物理
姓名 马任意 职称职务
邮箱 办公室
电话 个人主页
其他信息 研究方向岗位职责 黑洞吸积盘理论;高能辐射过程;宇宙学激波与高能宇宙射线
教育和工作经历 2001~2006 华中科技大学 博士
2006~2008 中科院上海天文台 博士后
2008~2010 韩国国立忠南大学 博士后
代表性文章或专著 1. Gong, X. L., Li, L. X., & Ma, R. Y. "A Disc-Corona Model for a Rotating Black Hole", Monthly Notices of the Royal Astronomical Society (Accepted)
2. Ma, R. Y., Ryu, D., & Kang, H. "Cosmic Rays Accelerated at Cosmological Shock Waves", J. Astrophys. Astr., 32, 301 (2011)
3. Edmon. P. P., Kang, H., Jones, T., & Ma, R. Y. "Non-thermal radiation from Type Ia supernova remnants", Monthly Notices of the Royal Astronomical Society, 414, 3521 (2011)
4. Yuan, F., Ma, R. Y., & Narayan, R. "A Simplified Global Solution for an Advection-dominated Accretion Flow", Astrophys. J., 679, 984 (2008)
5. Ma, R. Y., Yuan, F., & Wang, D. X. "Influence of the Magnetic Coupling Process on the Advection Dominated Accretion Flows around Black Holes", Astrophys. J., 671, 1981 (2007)
6. Ye, Y. C., Wang, D. X., & Ma, R. Y. "Magnetic coupling of a rotating black hole with advection-dominated accretion flows", New Astron., 12, 471 (2007)
7. Ma, R. Y., Wang, D. X., & Zuo, X. Q. "Influences of the magnetic coupling process on the spectrum of a disk covered by the corona", Astron. and Astrop., 453, 1 (2006)
8. Lei, W. H., Wang, D. X., & Ma, R. Y. "A Toy Model for Gamma-Ray Bursts in Type Ib/c Supernovae", Astrophys. J., 619, 420 (2005)
科研基金及项目 “Blazar伽玛辐射起源的重子模型”,国家自然科学基金主任基金项目
“Blazar的高能辐射机制及应用”,福建省自然科学基金面上项目
任教课程 大学物理
招生方向 荣誉奖励