'Charge exchange' presentation slideshows

Covering Solar-Wind Charge-Exchange from Every Angle with Chandra

Covering Solar-Wind Charge-Exchange from Every Angle with Chandra. Brad Wargelin Chandra X-Ray Center Smithsonian Astrophysical Observatory. Heliospheric Solar Wind Charge Exchange. Charge Exchange: The Forgotten Atomic Physics. Outline. Astrophysical charge exchange

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CP violation Lecture 6

CP violation Lecture 6. N. Tuning. Recap. u I. u. W. W. d,s,b. d I. Diagonalize Yukawa matrix Y ij Mass terms Quarks rotate Off diagonal terms in charged current couplings. Niels Tuning ( 3 ). CKM-matrix: where are the phases?.

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Status of Pentaquark Search

Status of Pentaquark Search. Valery Kubarovsky Rensselaer Polytechnic Institute / Jlab. Introduction Review of theoretical models Current Experimental Status Second generation experiments Conclusion . Introduction.

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PERSPECTIVES FOR HIGHLY POLARIZED ION SOURCES DEVELOPMENT

m. Muons, Inc. PERSPECTIVES FOR HIGHLY POLARIZED ION SOURCES DEVELOPMENT. Vadim Dudnikov, Muons, Inc., Batavia, IL USA. The XVth International Workshop on Polarized Sources, Targets and Polarimetry (PTSP 2013) the University of Virginia, Charlottesville, USA, September 2013. OUTLINE.

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Energetic Neutral Atom - ENA - Imaging Application to Planetary Research Joachim Woch, MPAE

Energetic Neutral Atom - ENA - Imaging Application to Planetary Research Joachim Woch, MPAE. Goal Principle Methods Instrumental Techniques Application - Results. view on plasma processes in a high-density, collisional, light emitting environment.

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Modeling Geomagnetic Storm Dynamics

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Ion sources for EICs

m. Muons, Inc. Ion sources for EICs. Vadim Dudnikov # , Muons, Inc., Batavia, IL USA. EIC Meeting at Stony Brook, January 10, 2010. m. Muons, Inc. Outline.

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Ionizing Radiation radioactivity measurements

Ionizing Radiation radioactivity measurements. High energy particles and photons that ionise atoms and molecules along their tracks in a medium are called ionizing radiation . For example, a, b, g, cosmic rays and X-rays are ionizing radiation.

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Why plasma processing? (1)

Why plasma processing? (1). Accurate etching of fine features. UCLA. The Coburn-Winters experiment. Ion bombardment greatly enhances chemical etching. UCLA. Why plasma processing? (2). Plasma enhanced chemical vapor deposition (PECVD) Sputtering Ashing. UCLA.

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Direct Reactions in/for Nuclear Astrophysics

Direct Reactions in/for Nuclear Astrophysics. Carlos Bertulani (University of Arizona). Nuclear Astrophysics. TeV/nucleon. keV/nucleon. ???. ???. Nuclear many-body problem: one of the hardest problems of all physics! Interactions are complicated Nucleons = composite particles

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Introduction to Plasma-Surface Interactions

Introduction to Plasma-Surface Interactions. Lecture 3 Atomic and Molecular Processes. Ionization and charge exchange. Neutral atoms entering the plasma from the boundary meet the plasma and are subject to ionization, excitation and charge exchange

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Exploration of Giant Planet Magnetospheres

Exploration of Giant Planet Magnetospheres. Fran Bagenal, University of Colorado. Jupiter Top Priority Polar Regions Multi-Spacecraft. Giant Planet Magnetospheres. Giant! Rotation Dominated Satellite plasma sources J&S Symmetric ~Dipolar Strong plasma production

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The abnormal wide annihilation line of solar flares

The abnormal wide annihilation line of solar flares. ShiChao TANG. Content. Observation Wide Line 3gamma/2gamma ratio Time profile Problem with the models. High Energy Resolution. http://hesperia.gsfc.nasa.gov/hessi/concept.htm. High Energy Resolution. Share et al 2003. Wide Line.

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by J.G. Cordey Based on lecture notes provided by M. Zarnstorff

Neutral Beams in TRANSP. by J.G. Cordey Based on lecture notes provided by M. Zarnstorff. The Monte Carlo technique is described in R.J. Goldston, D.C. McCune, et al. Journal of Computational Physics 43 61 (1981). General Model. Fast Neutral Propagation.

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Study on ? -A Reaction Cross Sections within CRPA

Study on ? -A Reaction Cross Sections within CRPA. Jeong-Yeon LEE and Yeong-Duk KIM Sejong University, KOREA. I. Why ? -A interactions?.

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Origin of Ion Cyclotron Waves in the Polar Cusp: Insights from Comparative Planetology

Origin of Ion Cyclotron Waves in the Polar Cusp: Insights from Comparative Planetology. Discovery by OGO-5 Ion cyclotron waves in other planetary magnetospheres Jupiter Saturn Theory Ion cyclotron waves at Mars and Venus Ion cyclotron waves observed by Polar Origin of ICWs in polar cusp?.

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A project of an experiment benefits from a full simulation of it (when possible)

CTMC Simulation of H-bar formation by charge exchange reaction with Ps G. Testera on behalf of C. Canali INFN Genoa AEGIS meeting CERN june 2006. A project of an experiment benefits from a full simulation of it (when possible) Several types of simulations are needed in AEGIS

196 views • 9 slides