Earl Scime

West Virginia University

Eberly Distinguished Professor & Chair of Physics

Department of Physics

 

P.O. Box 6315

 

Morgantown, WV 26506

 

Tel: (304) 293-3422 ext. 1437

 

Fax: (304)293-5732

VITAE

PUBLICATION LIST

CURRENT SCHEDULE

YOUTH ROBOTICS

 

 

Education

B.S., Florida State University, 1987

Ph.D., University of Wisconsin - Madison, 1992

 

Course Links

Physics 314 Modern Physics

Physics 781 Principles of Plasma Physics

Physics 782 Computational Plasma

LabWindows Example Code (compressed)

MATLAB Example Code (compressed)

Physics 784 Magnetohydrodynamics

 

Research Group Links

Research Team Photo

Plasma Physics at WVU
WVU Plasma Reunion at 2002 APS-DPP
2001 Helicon Sources Mini-Conference Online Poster Session

2007 Helicon Sources Mini-Conference Online Poster Session

 

The primary theme of the WVU plasma physics group is space-relevant plasma physics. My group has a number of experimental laboratory, experimental space, and theoretical research projects. The core of our experimental laboratory plasma physics program is a high-density helicon plasma source coupled to a large space simulation chamber [Large Experiment on Instabilities and Anisotropies (LEIA)]. The WVU Hot hELIcon eXperiment (HELIX) source operates in a steady-state mode and is unique in that it can operate over a wide range of driving frequencies (0.3-35 MHz) and exhibits relatively high ion temperatures. The ion temperatures in argon and helium plasmas are measured with a non-invasive, laser induced fluorescence diagnostic. Current research projects include the investigation of Alfven wave reflection and nonlinear interactions in high beta plasmas, coherent microwave scattering experiments to directly detect short wavelength, slow, waves in the edge of helicon sources, the development of new laser induced fluorescence schemes for argon and helium ions using tunable diode lasers, and the development of two-photon LIF schemes for the direct measurement of neutral hydrogen densities in fusion plasmas.

In collaboration with the Southwest Research Institute, Los Alamos National Laboratory, University of Southern California, and MIT, we participated in the launch of the world's first transmission grating based neutral atom imager on the IMAGE spacecraft in March 2000. This instrument directly detected and imaged neutral atoms emitted from the Earth's magnetosphere. With a single image, a neutral-atom "camera" can provide a detailed picture of the spatial distribution of the plasma trapped in the Earth's magnetosphere. The IMAGE mission has now ended and we have moved on to the TWINS mission. TWINS consists of two similar neutral atom cameras, each on different spacecraft.