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As an example, we shall present the energy spectrum and relative abundance for neon and discuss the implication of this result in the context of current models of acceleration and propagation of galactic cosmic rays.
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The model is based on a trapezoidal model of acceleration and deceleration.
The mechanism can be explained by the model of acceleration of senescence under Al stress.
The PCD was mitochondria dependence, and it can be explained by the model of acceleration of senescence under Al treatments (Zhan et al. [2013]).
With only one year of data, it is not possible to obtain reasonably accurate models of the acceleration.
Based on previous models of particle acceleration at CME-driven shocks, our simulation allows us to investigate various characteristics of energetic particles arriving at various distances from the sun.
This capability is important for various applications, including kinetic particles tracking in three dimensional vector fields, visualization (i.e. surface extraction) and extracting variables along one-dimensional curves such as field lines, streamlines and satellite trajectories, etc. Particular examples are models for acceleration of solar energetic particles (SEPs) along magnetic field-lines.
The sensing and modeling of joint acceleration via linear accelerometers is dealt from the viewpoint of practical implementation.
A dynamical time-dependent model of particle acceleration at coronal mass ejection (CME) driven shock waves is presented.
Point-model of CT acceleration in a co-axial electrode is solved to optimize the electrode geometry and the power supplies.
DOI: http://dx.doi.org/10.7554/eLife.02407.017 10.7554/eLiFigure07.018 Figure 4 figure supplement 1. Monte-Carlo modeling of the acceleration and the termination hypotheses.
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