Department of Physics, South China Univ. of Tech. Properties of Neutron Star and its oscillations 2011.11 collaborators Bao-An Li, William Newton, Plamen.
Plasma Presentation2
Martian and terrestrial Satellite Magnetic Data: Crustal magnetization and downward continuation models Kathy Whaler University of Edinburgh, UK GEST Visiting.
ESS 200C Lecture 12 Planetary Magnetospheres. We have studied the Earth’s magnetosphere in great detail for over 40 years and think we have developed.
Investigation Overview, Scherrer, Page 1SDO Science Writers Workshop – 16 Dec 2009 HMI Investigation Overview Philip Scherrer HMI Principal Investigator.
A Debris Disk Around an Isolated Young Neutron Star Deepto Chakrabarty Zhongxiang Wang David L. Kaplan Kavli Institute for Astrophysics and Space Research.
The Atmospheric Imaging Assembly Measuring the Sun’s Surface, Chomosphere, Transition Region, and Corona using visible and extreme Ultra- violet light.
(Some of the possible) Astrophysical origins of high energy cosmic rays Diego F. Torres [email protected] Lawrence Livermore Lab. California, 94550,
R.L. Geng ALCPG2011, 3/19-23,2011 1 Cavity Process and General R&D Plan and Proposal Rongli Geng Jefferson Lab & GDE Linear Collider Workshop of the Americas.
SRF CAVITY GEOMETRY OPTIMIZATION FOR THE ILC WITH MINIMIZED SURFACE E.M. FIELDS AND SUPERIOR BANDWIDTH The Cockcroft Institute of Accelerator Science and.
Why was the Sun so quiet?
Crustal magnetization
