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SteadyState Image Processing
, 2001
"... This paper presents a new approach to the application mode of image processing operators, the socalled steadystate image processing. The approach reminds a steadystate genetic processing of images by considering each pixel of the image as an individual. So, some pixels are selected, processed and ..."
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of texture segmentation. Steadystate image processing can be considered a way of processing images, which is deeply inspired by genetic algorithms. 2001 Elsevier Science B.V. All rights reserved. Keywords: Soft image processing; Linear pixel shuffling; Autopoiesis; Steadystate genetic algorithms 1.
Graphical Representation of SteadyState Trophic Ecosystem Models*
"... PAULY, D. and V. CH~ISTENSEN. 1993. Graphical representation ofsteadystate trophic ecosystem models, p.2028. In V. Christensen and D. Pauly (eds.) Trophic models ofaquatic ecosystems. ICLARM Conf. Proc. 26,390 p. The traditional method of representing steadystate ecosystem models, usually by scat ..."
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PAULY, D. and V. CH~ISTENSEN. 1993. Graphical representation ofsteadystate trophic ecosystem models, p.2028. In V. Christensen and D. Pauly (eds.) Trophic models ofaquatic ecosystems. ICLARM Conf. Proc. 26,390 p. The traditional method of representing steadystate ecosystem models, usually
SteadyState Bifurcations in Reversible Equivariant Systems
"... . We present results on generic \separable" bifurcations of equilibria of equivariant dynamical systems with nite symmetry groups and timereversing symmetries. These bifurcation problems are reduced to standard equivariant bifurcation problems using equivariant transversality theory. For ea ..."
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and further results will be published elsewhere. 1. Introduction Let V be a vector space, G a nite group and a linear representation of G on V . Consider also a representation : G ! f1g and dene = . We say that a smooth mapping f : V ! V is Greversibleequivariant if f((g)x) = (g)f(x) = (g)(g)f(x) 8g
LHD Diagnostics Toward SteadyState Operation
"... Abstract—The large helical device (LHD) is the world largest helical system having all superconducting coils. After completion of LHD in 1998, six experimental campaigns have been carried out successfully. The maximum stored energy, central electron temperature, and volume averaged beta value are 1. ..."
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.16 MJ, 10 keV, and 3.2%, respectively. The confinement time of the LHD plasma appears to be equivalent to that of tokamaks. One of the most important missions for LHD is to prove steadystate operation, which is also significant to international thermonuclear experimental reactor (ITER) and to future
Iron Indices and Intravenous Ferumoxytol: Time to SteadyState
"... Anemia is prevalent in patients withstage V chronic kidney disease (CKD) undergoing hemodialysis (HD) because of the deficiency of endogenous erythropoietin. In HD patients treated with an erythropoiesisstimulating agent (ESA), relative iron deficiency is the most common cause of anemia.13 It oft ..."
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Anemia is prevalent in patients withstage V chronic kidney disease (CKD) undergoing hemodialysis (HD) because of the deficiency of endogenous erythropoietin. In HD patients treated with an erythropoiesisstimulating agent (ESA), relative iron deficiency is the most common cause of anemia.13 It of
Estimation of steadystate basic parameters of stars B.V.Vasiliev
, 2000
"... Coming from the requirement of a minimum of total energy of celestial bodies, their basic parameters are calculated. The steadystate values of mass, radius, and temperature of stars and white dwarfs, as well as masses of pulsars are obtained. The luminosity and giromagnetic ratio of celestial bodie ..."
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Coming from the requirement of a minimum of total energy of celestial bodies, their basic parameters are calculated. The steadystate values of mass, radius, and temperature of stars and white dwarfs, as well as masses of pulsars are obtained. The luminosity and giromagnetic ratio of celestial
Estimation of steadystate basic parameters of stars B.V.Vasiliev
, 2000
"... From a minimum of total energy of celestial bodies, their basic parameters are obtained. The steadystate values of mass, radius, and temperature of stars and white dwarfs, as well as masses of pulsars are calculated. The luminosity and giromagnetic ratio of celestial bodies are estimated. All the o ..."
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From a minimum of total energy of celestial bodies, their basic parameters are obtained. The steadystate values of mass, radius, and temperature of stars and white dwarfs, as well as masses of pulsars are calculated. The luminosity and giromagnetic ratio of celestial bodies are estimated. All
Some Kinetic and SteadyState Properties of Sodium Channels after Removal of Inactivation
"... ABSTRACT To study the kinetic and steadystate properties of voltagedependent sodium conductance activation, squid giant axons were perfused internally with either pronase or Nbromoacetamide and voltage clamped. Parameters of activation, ~'m and gNa(V), and deactivation, r were measured and c ..."
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ABSTRACT To study the kinetic and steadystate properties of voltagedependent sodium conductance activation, squid giant axons were perfused internally with either pronase or Nbromoacetamide and voltage clamped. Parameters of activation, ~'m and gNa(V), and deactivation, r were measured
STEADYSTATE ELECTROSTATIC LAYERS FROM WEIBEL INSTABILITY IN RELATIVISTIC COLLISIONLESS SHOCKS
, 2005
"... Preprint typeset using LATEX style emulateapj v. 10/10/03 ..."
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