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141
Analysis of the early stage of thermal runaway
, 1985
"... It is shown that a variable grouping containing a logarithmic timedependent factor is required for the development of a coordinateperturbation expansion which realistically describes the spatially varying thermalrunaway process. The resulting solution is in good agreement with careful numerical c ..."
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Cited by 11 (0 self)
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It is shown that a variable grouping containing a logarithmic timedependent factor is required for the development of a coordinateperturbation expansion which realistically describes the spatially varying thermalrunaway process. The resulting solution is in good agreement with careful numerical
Runaway Acceleration of LineDriven Winds: . . .
, 2002
"... Observations and theory suggest that linedriven winds from hot stars and luminous accretion disks adopt a unique, critical solution that corresponds to maximum massloss rate. We analyze the numerical stability of the infinite family of shallow wind solutions, which resemble solar wind breezes, and ..."
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, and their transition to the critical wind. Shallow solutions are subcritical with respect to radiative (or Abbott) waves. These waves can propagate upstream through shallow winds at high speeds. If the waves are not accounted for in the Courant time step, numerical runaway results. The outer boundary condition
ANALYSIS OF THE EARLY STAGE OF THERMAL RUNAWAY
, 1984
"... It is shown that a variable grouping containing a logarithmic timedependent factor is required for the development of a coordinateperturbation expansion which realistically describes the spatially varying thermalrunaway process. The resulting solution is in good agreement with careful numerical c ..."
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It is shown that a variable grouping containing a logarithmic timedependent factor is required for the development of a coordinateperturbation expansion which realistically describes the spatially varying thermalrunaway process. The resulting solution is in good agreement with careful numerical
A Multiwavelength Study of the Runaway Binaries
"... Abstract: The runaway Otype binaries HD14633 and HD15137 were likely ejected from the cluster of their birth by supernovae explosions in close binaries. Here we present recent optical spectra to update the orbital solutions of the binaries and study the physical parameters of the O star primaries. ..."
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Abstract: The runaway Otype binaries HD14633 and HD15137 were likely ejected from the cluster of their birth by supernovae explosions in close binaries. Here we present recent optical spectra to update the orbital solutions of the binaries and study the physical parameters of the O star primaries
Runaway electrons Relativistic Plasma Kinetic
, 2013
"... Synchrotron emission from runaway electrons may be used to diagnose plasma conditions during a tokamakdisruption, but solving this inverse problem requires rapid simulation of the electrondistribution function and associated synchrotron emission as a function of plasma parameters. Here we detail a f ..."
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primary and secondary runaway electron generation are included. For cases in which primary generation dominates, a timeindependent formulation of the problem is described, requiring only the solution of a single sparse linear system. In the limit of dominant secondary generation, we present the first
Runaway Charged Particles and Center Manifolds
, 1998
"... We consider the coupled MaxwellLorentz equations for a single charge with a rigid charge distribution subject to slowly varying external potentials. In the adiabatic limit, to lowest order, the motion of the charge is governed by an effective Hamiltonian. In the next order we obtain, as a small ..."
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Cited by 2 (2 self)
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small correction, the radiation reaction containing \Delta\Delta\Delta q terms. This equation has a stable center manifold and the true solution stays close to the center manifold. The motion on the center manifold is governed by a novel second order equation which contains "
On the Mass Distribution of Planetesimals in the Early Runaway Stage
, 1998
"... We derive the stationary distribution of the mass of planetesimals from the coagulation equation under the assumption of energy equipartition. In the threedimensional case, we found that the stationary solution is expressed as n(m) / m 08=3 , where n is the surface number density and m is the mas ..."
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Cited by 5 (0 self)
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dimensional case, the stationary solution exists but cannot be realized in a finite time. This difference is the direct consequence of the fact that runaway growth takes place in three dimensions, but not in two dimensions. Key words: Planetary Formation, Planetary Accretion, Runaway Growth, Planetesimals 1
Control of consolidation in neural networks: avoiding runaway effects
 Connection Science
, 2003
"... Abstract. Consolidation has been implemented in two ways: as straight rehearsal of patterns or as pseudorehearsal, in which pseudoitems are created by sampling attractors or input–output combinations from the network. Although both implementations have been investigated by several authors, few have ..."
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Cited by 9 (4 self)
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is analysed, and three solutions are explored. Suppressing transmission in the connections in which consolidation takes place is shown to work best. Placing bounds on connections or unlearning attractors also alleviates runaway consolidation, though less effectively so.
A Spectroscopic Study of Field and Runaway OB Stars
, 2006
"... Identifying binaries among runaway O and Btype stars offers valuable insight into the evolution of open clusters and close binary stars. Here we present a spectroscopic investigation of 12 known or suspected binaries among field and runaway OB stars. We find new orbital solutions ..."
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Identifying binaries among runaway O and Btype stars offers valuable insight into the evolution of open clusters and close binary stars. Here we present a spectroscopic investigation of 12 known or suspected binaries among field and runaway OB stars. We find new orbital solutions
Hazard of Runaway of Nitration Processes in Nitrocompounds Production
"... Abstract: Hazard of runaway of nitration processes in nitrocompounds production was investigated. Temperature rise in DNT nitration mixes under near adiabatic conditions was measured, and derivative dT/dτ was computed. Heat evolution rate caused by nitration (primary reaction) and oxidation (seconda ..."
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Abstract: Hazard of runaway of nitration processes in nitrocompounds production was investigated. Temperature rise in DNT nitration mixes under near adiabatic conditions was measured, and derivative dT/dτ was computed. Heat evolution rate caused by nitration (primary reaction) and oxidation
Results 1  10
of
141