蒋苏云

作者:来源:发布时间:2017-04-14

个人简介

蒋苏云,女,1956年9月出生,江苏省常州(县市)人,现为
浙江师范大学数理信息学院教授。


学习经历

1978.3-1982.1  云南大学物理系获理学学士,物理专业;

1988.9-1992.4  中国科学院云南天文台获理学硕士学位,天体物理专业;

1992.4-1995.11 中国科学院云南天文台获理学博士学位,天体物理专业;

1996.8-1998.4,中国科学技术大学天体物理中心做博士后。


工作简历

1974.9-1977.3   云南省丽江县黄山公社下乡知青;

1977.3-1978.3   云南省丽江地区电机厂铸工;

1982.1-1988.9   中国科学院云南天文台从事科研;

1995.11-1996.8   中国科学院云南天文台从事科研;

1998.4-1998.12  中国科学技术大学天体物理中心任教;

1998.12-至今   浙江师范大学数理信息学院任教;

助工(1983.5)/助研(1989.7)/副教授(1997.6)教授(2005.11)


人才梯队、荣誉

浙江省151第二层次入选者(1999.12);

浙江省高校中青年学科带头人入选者(1999.12);

中国科学院优秀博士研究生奖(1994.12);

浙江师范大学校“三育人”工作先进个人奖(2003.12)。


研究领域及成果

长期从事天体物理学专业领域的研究,在该领域取得一定成绩,在《Astronomy and Astrophysics》、《中国科学(A辑)》、《Chinese Journal of Astronomy and Astrophysics》、《天体物理学报》、《天文学报》等杂志上发表论文30余篇。

代表性论文、论著

1.论文“初始质量为7MAGB星质量喷射和热脉动” 1995年7月发表于《天文学和天体物理学》第293期;

2.论文“湍流压对红巨星和AGB 星的影响I.内部结构和演化” 1997年1月发表于《天文学和天体物理学》第317期;

3.论文“湍流压对红巨星和AGB 星的影响II.产生强大星风物质损失的机理” 1997年1月发表于《天文学和天体物理学》第317期;

4.论文“湍流压对中小质量恒星后期演化的影响 (I).湍流压、物态方程及热力学量的计算” 1997年10月发表于《中国天文学和天体物理学》第21卷第4期;

5.论文“湍流压对中小质量恒星后期演化的影响 (II).湍流压对内部结构和演化的影响” 1998年4月发表于《中国天文学和天体物理学》第22卷第2期;

6.论文“AGB星氦燃烧壳层源出现非稳定热核反应的判据” 2006年4月发表于《中国天文学和天体物理学》第30卷第2期

7.论文“8M恒星演化过程中湍流应力作用效果的分析” 2006年4月发表于《中国天文学和天体物理学》第30卷第2期;

8.论文“中等质量恒星星风物质损失的机制” 2012年4月发表于《中国天文学和天体物理学》第36卷第2期;

9.论文“中等质量恒星在赫罗图中由E-AGB星进入TP-AGB星的分界点” 2012年1月发表于《中国天文学和天体物理学》第36卷第1期

代表性科研项目
  1. 1994-1996, 云南省自然科学基金一般项目-“AGB星产生超星风及热脉动机理研究”;
  2. 1997-1998, 国家自然科学基金一般项目-“红巨星、AGB星强大星风物质损失的机理研究”;
  3. 2001-2003, 国家自然科学基金一般项目-“矮活动星系的星族合成”;
  4. 2004-2005, 浙江省自然科学基金一般项目-“湍流压效应对恒星结构和演化的影响”
成果获奖

项目《230—300MHz太阳米波数字声光频谱仪》获1986年中国科学院科学技术进步二等奖


近三年教学情况

为本科生主讲课程有《热学》、《大学物理学》、《普通天文学》,指导本科生论文30篇;为研究生开设《天体物理学》、《恒星物理学》、《太阳物理学导论》等课程,指导培养硕士研究生6名。


Profile

Jiang Suyun, 1956 born in Changzhou city in Jiangsu Province in September. now she is the professor of Zhejiang Normal University College of mathematical and information


Education Background

1978.3-1982.1   Received the Bachelor of Science in Physics Department of Yunnan University, majoring in physics;

1988.9-1992.4   The Yunnan Observatory of Chinese Academy of Sciences, master of Science in professional, astrophysics;

1992.4-1995.11  Received a doctor degree in science from the Yunnan Observatory of Chinese Academy of Sciences, astrophysics professional;

1996.8-1998.4  University of Science & Technology China Center for Astrophysics postdoctoral.


Work Experiences

1974.9—1977.3   The commune of Lijiang County of Yunnan province Mount Huangshan educated youth;

1977.3 —1978.3   Lijiang area of Yunnan Province Motor Factory Foundry;

1982.1—1988.9   The Yunnan Observatory of Chinese Academy of Sciences, engaged in scientific research;

1995.11—1996.8  The Yunnan Observatory of Chinese Academy of Sciences, engaged in scientific research;

1998.4 —1998.12    At the University of Science & Technology China Center for astrophysics;

1998.12—up to now  At the Zhejiang Normal University School of mathematical information;

 Assistant Engineer(1983.5)/ Assistant Research Fellow(1989.7)/ Associate Professor(1997.6)Professor(2005.11)


Honorable Titles and Awards:

Zhejiang province 151 second level candidates(1999.12);

Zhejiang Province young academic leaders in University(1999.12);

China's outstanding doctoral Academy Award(1994.12)

Zhejiang Normal University School of "three aspects of education" advanced individual award(2003.12)


Research Field and Achievements

Research in Astrophysics professional engaged in long-term, certain achievements have been made in this field, in the "Astronomy and Astrophysics", "science in China (series A)", "Chinese Journal of Astronomy and Astrophysics", "Astrophysical Journal", "Chinese Journal of astronomy" magazine published more than 30 papers.


Representative Works

1.The paper “ On the mass ejection and thermal pulses of an AGB star with an initial mass of 7M” in 1995 July published in the " Astronomy and Astrophysics",Volume 293.

2. The paper “The effect of turbulent pressure on the red giants and AGB stars I.On the internal structure and evolution” in 1997 January published in the " Astronomy and Astrophysics",Volume 317.

3. The paper “ The effect of turbulent pressure on the red giants and AGB stars II.On the mechanism powering the strong stellar winds” in 1997 January published in the " Astronomy and Astrophysics",Volume 317.

4. The paper “The influence of turbulent pressure on the late stages of evolution of low- and intermediate-mass star.(I).Calculations for turbulent pressure,the equation of state and the thermodynamic quantities” in 1997 October published in the "Chinese Astronomy and Astrophysics ",Volume 21, Issue 4.

5. The paper “The influence of turbulent pressure on the late stages of evolution of low- and intermediate-mass stars. II. The effect on the internal structure and evolution” in 1998 April published in the "Chinese Astronomy and Astrophysics ",Volume 22, Issue 2.

6. The paper “The criterion of appearance of unsrable thermonuclear reaction in the helium burning shell on AGB stars” in 2006 April published in the "Chinese Astronomy and Astrophysics ",Volume 30, Issue 2.

7. The paper “An analysis of the effect of turbulent stress on the evolution of an 8MStar” in 2006 April published in the "Chinese Astronomy and Astrophysics ",Volume 30, Issue 2.

8. The paper “The Demarcation Point from E-AGB Stars to TP-AGB Stars in HR Diagram for Medium-mass Stars”in 2012 January published in the "Chinese Astronomy and Astrophysics ",Volume 36, Issue 1.

9. The paper “Mechanism of Mass Loss of Stellar Wind for Medium-mass Stars” in 2012 April published in the "Chinese Astronomy and Astrophysics ",Volume 36, Issue 2.

Research Projects

1. 1994 – 1996, the Yunnan Province Natural Science Fund Project - " AGB stars superstar wind and thermal pulse mechanism research";

2. 1997 – 1998, the National Natural Science Fund Project -"the mechanism of "red giant star, AGB Star strong wind material loss ;

3. 2001–2003, National Natural Science Fund Project - "dwarf galaxy population synthesis activity";

4. 2004 – 2005, the Zhejiang Province Natural Science Fund Project - "turbulent pressure effect on the stellar structure and evolution of stars "

Awards

The project "230 - 300MHz solar meter wave digital acousto optical spectrometer" won the two prize in 1986 the Chinese Academy of science and technology progress.


Teaching and Supervision during Last 3 Years

For undergraduate courses have a "heat", "university physics", "general astronomy", guide the students papers 30; for graduate students "astrophysics", "stellar physics", "sun" Introduction to physics curriculum, instruction training postgraduates 6.