Two Dimensional PIC Simulation of Anode Foil Evolution in Axially-Extracted Vircator

2007 ◽  
Author(s):  
G. Singh ◽  
S. Chaturvedi
Keyword(s):  
Two Dimensional ◽  
Pic Simulation ◽  
Anode Foil

Two-Dimensional Hybrid-PIC Simulation of Magnetic Sail Including Interplanetary Magnetic Field

2012 ◽  
Vol 60 (1) ◽  
pp. 31-39
Author(s):  
Masaharu MATSUMOTO ◽  
Yoshihiro KAJIMURA ◽  
Hideyuki USUI ◽  
Ikkoh FUNAKI ◽  
Iku SHINOHARA
Keyword(s):  
Magnetic Field ◽  
Interplanetary Magnetic Field ◽  
Two Dimensional ◽  
Pic Simulation

scholarly journals Two-dimensional PIC simulation of atomic clusters in intense laser fields

2004 ◽  
Vol 22 (2) ◽  
pp. 137-145 ◽  
Author(s):  
F. GRESCHIK ◽  
H.-J. KULL
Keyword(s):  
Laser Intensity ◽  
Laser Pulses ◽  
Atomic Clusters ◽  
Intense Laser ◽  
Electron Mass ◽  
Two Dimensional ◽  
Intense Laser Fields ◽  
Pic Simulation ◽  
Intense Laser Pulses ◽  
Cylindrical Plasma Column

Collective absorption of intense laser pulses by atomic clusters is studied by PIC simulations. The cluster is modeled in two-dimensional calculations as a cylindrical plasma column with a diameter of D = 6.4 nm and an initial electron density of ne0 = 1023 cm−3. The frequency and intensity dependence of absorption is discussed. It is found that nonresonant absorption by electron emission increases as a power law with the laser intensity. The absorbed energy per electron reaches a maximum of about Wmax = mωp2D2 (ωp: plasma frequency, m: electron mass) at the intensity where ionization saturates.

Spectrophotometric measurements of objective-prism spectra

1966 ◽  
Vol 24 ◽  
pp. 118-119
Author(s):  
Th. Schmidt-Kaler
Keyword(s):  
Progress Report ◽  
Two Dimensional ◽  
Objective Prism ◽  
Made In

I should like to give you a very condensed progress report on some spectrophotometric measurements of objective-prism spectra made in collaboration with H. Leicher at Bonn. The procedure used is almost completely automatic. The measurements are made with the help of a semi-automatic fully digitized registering microphotometer constructed by Hög-Hamburg. The reductions are carried out with the aid of a number of interconnected programmes written for the computer IBM 7090, beginning with the output of the photometer in the form of punched cards and ending with the printing-out of the final two-dimensional classifications.

Introductory paper

1966 ◽  
Vol 24 ◽  
pp. 3-5
Author(s):  
W. W. Morgan
Keyword(s):  
Line Intensity ◽  
Classification Scheme ◽  
Two Dimensional ◽  
Spectral Classification ◽  
Dimensional Array ◽  
Rr Lyrae ◽  
Metallic Line ◽  
Introductory Paper ◽  
Parameter Varying ◽  
Definition Of

1. The definition of “normal” stars in spectral classification changes with time; at the time of the publication of theYerkes Spectral Atlasthe term “normal” was applied to stars whose spectra could be fitted smoothly into a two-dimensional array. Thus, at that time, weak-lined spectra (RR Lyrae and HD 140283) would have been considered peculiar. At the present time we would tend to classify such spectra as “normal”—in a more complicated classification scheme which would have a parameter varying with metallic-line intensity within a specific spectral subdivision.

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