'Growth time' presentation slideshows

Jan 2004

Head-Tail and Coupled-Bunch Electron Cloud Instability and Benchmarking Mauro Pivi NLC Division SLAC. Jan 2004. Motivations and goals.

500 views • 39 slides

Resistive Wall Mode (RWM) Study on JT-60U

JSPS-CAS Core University Program 2008 in ASIPP Plasma and Nuclear Fusion Feb. 16-21, 2009 in ASIPP. Resistive Wall Mode (RWM) Study on JT-60U. Go Matsunaga ???? Japan Atomic Energy Agency, Naka, Japan. Outline. Introduction Current driven RWM in OH plasmas RWM in high- b plasmas

436 views • 32 slides

The formation of stars and planets

428 views • 30 slides

The formation of stars and planets

431 views • 30 slides

The formation of stars and planets

400 views • 30 slides

COMPLEX FLOW OF NANOCONFINED POLYMERS

COMPLEX FLOW OF NANOCONFINED POLYMERS. Connie B. Roth, Chris A. Murray and John R. Dutcher Department of Physics University of Guelph Guelph, Ontario, Canada N1G 2W1. OUTLINE. instabilities in freely-standing liquid films hole growth in freely-standing PS films

422 views • 30 slides

COMPLEX FLOW OF NANOCONFINED POLYMERS

COMPLEX FLOW OF NANOCONFINED POLYMERS. Connie B. Roth, Chris A. Murray and John R. Dutcher Department of Physics University of Guelph Guelph, Ontario, Canada N1G 2W1. OUTLINE. instabilities in freely-standing liquid films hole growth in freely-standing PS films

308 views • 30 slides

Super Massive Black Holes

Super Massive Black Holes. The Unknown Astrophysics of their initial formation. Characteristics of SBMH. Crit = light cone loss A = accretion radius Coll = stellar disruption radius E = eddington radius; radiation pressure limits accretion; more efficient with larger G T = tidal radius

324 views • 21 slides

Super Massive Black Holes

Super Massive Black Holes. The Unknown Astrophysics of their initial formation. Characteristics of SBMH. Crit = light cone loss A = accretion radius Coll = stellar disruption radius E = eddington radius; radiation pressure limits accretion; more efficient with larger G T = tidal radius

334 views • 21 slides

Smaller (vertical) beta function Long bunch spacing

Wi =Length_element/ Length_section Wi=0 if ion is unstable. Both growth rate and tune-shift are small if there is a. Smaller (vertical) beta function Long bunch spacing. Peak growth rate of FII for CO+. Pwiggler= 2.0nTorr ; Plong_straight = 0.1nTorr P_arc= 0.5nTorr.

244 views • 15 slides

Smaller (vertical) beta function Long bunch spacing

Wi =Length_element/ Length_section Wi=0 if ion is unstable. Both growth rate and tune-shift are small if there is a. Smaller (vertical) beta function Long bunch spacing. Peak growth rate of FII for CO+. Pwiggler= 2.0nTorr ; Plong_straight = 0.1nTorr P_arc= 0.5nTorr.

280 views • 15 slides

Experimental Components

Experimental Components. Experiment to test hypothesis *overall question*. Must include both experiments below. Control Experiment- This experiment includes what you are comparing to. You either remove the independent variable or test what you have always done in the past.

219 views • 13 slides

SuperDARN and reversed flow events in the cusp

SD2011. SuperDARN and reversed flow events in the cusp. K. Oksavik 1 , J. Moen 1,2 , E. H. Rekaa 2 , H. C. Carlson 3 , and M. Lester 4 1) UNIS, Longyearbyen, Norway 2) Department of Physics, Univ. Oslo, Oslo, Norway 3) CASS, Utah State University, USA

225 views • 12 slides

Motivation and Overview

100 views • 1 slides