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Year of China Lecture Series: The Increasing Role of China in Global Food Security - Shenggen Fan

Year of China Lecture Series: The Increasing Role of China in Global Food Security

Shenggen Fan, Director General, International Food Policy Research Institute

 

Monday, March 26, 2012

6:00 - 7:30pm

Whitehall Classroom Building Room 118

Date:
Location:
Whitehall Classroom Building Room 118

Year of China Lecture Series: When is the Postcolonial Imperial? - Shu-mei Shih

Year of China Lecture Series: When is the Postcolonial Imperial? Chinese Intellectuals and the Tibet Question

Shu-mei Shih, Professor of Asian Languages and Cultures & Asian American Studies, UCLA

6:00 - 7:40pm, Thursday March 22

Whitehall Classroom Building Room 118

Date:
Location:
Whitehall Classroom Building Room 118

Year of China Film Series - Autumn Gem (秋瑾)

 

April 10, 2012 - 6:00pm
Whitehall Classroom Bldg 118

Autumn Gem (秋瑾)http://autumn-gem.com/ Autumn Gem is a documentary about China’s first feminist, Qiujin. Qiujin (1875-1907) defied tradition to become the leader of a revolutionary army. She was the first woman to lead an armed uprising against the Qing dynasty government, for which she was arrested and executed. Autumn Gem was released in 2009.

Date:
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Location:
Whitehall Classroom Building Room 118

Ernie Yanarella & Richard Levine, Year of China Lecture Series

 

Year of China Lecture Series, featuring:

Ernie Yanarella - Professor and Chair, Department of Political Science

Richard Levine - Emeritus Professor, Architecture

A Tale of Two Projects: Hangbaiyu and SUCCESS

April 5, 2012

Whitehall Classroom Building Room 118

6:00-7:40pm

Free and open to the public

Date:
-
Location:
Whitehall Classroom Building Room 118

Demolition (拆迁 ) & discussion with the director

 

April 3, 2012 - 6:00pm
Whitehall Classroom Bldg 118

Demolition(拆迁 ) & discussion with the director

http://hcl.harvard.edu/hfa/films/2009mayjun/sniadecki.html

Demolition explores the impacts of migrant labor and the urban experience by focusing on the city of Chengdu, the capital of Sichuan province. Director J.P. Sniadecki examines the interactions between the members of China’s floating population of migrant workers and the residents of Chengdu as well as the booming construction industry in China.

Date:
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Location:
Whitehall Classroom Building Room 118

Astro Seminar: Gururaj Wagle

Modeling the Cirrus Clouds



Abstract:



The cirrus clouds are mainly diffuse or translucent clouds, with typically

a very low visual extinction. But such clouds may have dense molecular cores.

These cores could be precursors to star formation and are very good candidates

to study early phases of stellar evolution. Despite of the apparent simplicity of

these regions, the observations of the dense gas tracers contradict with the

models and hence suggesting a gap in our understanding of these regions.

Polaris Flare is a high latitude cirrus cloud, with several star-less cores. A

translucent molecular cloud MCLD 123.5+24.9 is one of the denser regions of

the Polaris cirrus complex, located in the direction near the celestial North Pole.

I am going to discuss the models of this region using Cloudy with the help of

CO transition line observations and recent Herschel observations from the

continuum dust emission.

Date:
-
Location:
179 Chem-Phys Bldg

Astro Seminar: Ye Wang

Quasar Spectral Energy Distributions and the Effects of Intervening Clouds



Abstract:



The nature of the Broad Line Region (BLR) of Active Galactic Nuclei (AGN) is an area of

vigorous debate. The geometry of the BLR clouds is also uncertain. I will first present

the current model of AGNs and BLR. Then I will review recent work on the X-ray time

variability of Mrk 766, a Seyfert 1 galaxy.  I will then introduce a new geometry for

the BLR clouds. This new geometry, which we call the intervening BLR clouds model,

has BLR clouds along our line of sight. These intervening clouds generate a depression

at ~900Å to ~1200Å. Observations of Mrk 766 and other AGNs suggest that intervening

clouds may exist in most AGNs. The real SED of the AGNs in that wavelength range may

be higher than we now suppose due to the depression made by intervening clouds.

Date:
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Location:
179 Chem-Phys Bldg
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