
Resume
... Led process line in process development, device fabrication and inline testing of a collaboration project. Developed low temperature low stress high quality PECVD processes for flexible display applications. Optimized plasma etching processes for low temperature high performance polysilicon TFT fabr ...
... Led process line in process development, device fabrication and inline testing of a collaboration project. Developed low temperature low stress high quality PECVD processes for flexible display applications. Optimized plasma etching processes for low temperature high performance polysilicon TFT fabr ...
PPT
... that it has a buoyancy then continue to move up. • Denser plasma which pushed down is heavier than surrounding plasma so that it has stronger gravity force then continue to down. • Therefore, both dense and lighter plasmas are mixing each other. • This is so-called Rayleigh-Taylor instability ...
... that it has a buoyancy then continue to move up. • Denser plasma which pushed down is heavier than surrounding plasma so that it has stronger gravity force then continue to down. • Therefore, both dense and lighter plasmas are mixing each other. • This is so-called Rayleigh-Taylor instability ...
Magnetic field generation in weak-line T Tauri stars
... of avoiding the singularity at the origin of the coordinate system, it does not allow detailed radial profiles of density, magnetic diffusivity and other relevant parameters. We use averaged values for these quantities as well as for their gradients where necessary. Moreover, it is not very convenie ...
... of avoiding the singularity at the origin of the coordinate system, it does not allow detailed radial profiles of density, magnetic diffusivity and other relevant parameters. We use averaged values for these quantities as well as for their gradients where necessary. Moreover, it is not very convenie ...
The strongest magnetic fields in the universe: how strong can they
... Very formally, except as for inclusion of relativistic effects, Equation (4) provides a model equation for a limiting field in dependence on any given fundamental length scale c . Under this simplifying assumption the critical magnetic field Bc scales simply with the inverse square of the correspon ...
... Very formally, except as for inclusion of relativistic effects, Equation (4) provides a model equation for a limiting field in dependence on any given fundamental length scale c . Under this simplifying assumption the critical magnetic field Bc scales simply with the inverse square of the correspon ...
Magnetic fields in the Universe
... electron column between us and the source and other backgrounds. There is limited agreement that in clusters and superclusters the field is about .1µG and in the Universe perhaps between 10-9 to 10-11 G, though this is not established. The Faraday rotation and synclotron radiation requires knowledge ...
... electron column between us and the source and other backgrounds. There is limited agreement that in clusters and superclusters the field is about .1µG and in the Universe perhaps between 10-9 to 10-11 G, though this is not established. The Faraday rotation and synclotron radiation requires knowledge ...
Solar-B - to Nobeyama Radio Observatory
... - Stellar Structure / Evolution - Dynamo Mechanism (Cosmic Magnetism) 2. Corona: a Prototype for Superhot Astrophysical Plasma - Why is the corona so hot? - Coronal Structure / Dynamics - Sudden Energy Release and Particle Acceleration * Key Word: Magnetic Reconnection 3. Factors Controlling the Spa ...
... - Stellar Structure / Evolution - Dynamo Mechanism (Cosmic Magnetism) 2. Corona: a Prototype for Superhot Astrophysical Plasma - Why is the corona so hot? - Coronal Structure / Dynamics - Sudden Energy Release and Particle Acceleration * Key Word: Magnetic Reconnection 3. Factors Controlling the Spa ...
Plasma Seminar, April 13, 2015 "The Magnetized Dusty Plasmas
... • Observed in a 4 T, rf parallel-plate device at MPE by Schwabe and Konopka (PRL 106, 215004, 2011) • As the magnetic field was increased, the plasma broke up into filaments aligned along B. • The motion of the particles in the discharge changed dramatically from a collective rotation in moderate fi ...
... • Observed in a 4 T, rf parallel-plate device at MPE by Schwabe and Konopka (PRL 106, 215004, 2011) • As the magnetic field was increased, the plasma broke up into filaments aligned along B. • The motion of the particles in the discharge changed dramatically from a collective rotation in moderate fi ...
A Rigid-Field Hydrodynamics approach to modelling the
... subject to pressure, radiative, gravitational and centrifugal forces. We solve these equations numerically for a large ensemble of field lines to build up a three-dimensional time-dependent simulation of a model star with parameters similar to the archetypal Bp star σ Ori E. Since the flow along eac ...
... subject to pressure, radiative, gravitational and centrifugal forces. We solve these equations numerically for a large ensemble of field lines to build up a three-dimensional time-dependent simulation of a model star with parameters similar to the archetypal Bp star σ Ori E. Since the flow along eac ...