D Jung, L Yin, BJ Albright, DC Gautier… - Physical Review Letters, 2011 - APS ... In addition, protons are here not affected by this acceleration mechanism, as they are mostly evacuated from the target by the time the accelerationphase starts due to the very low atomic content of protons in the target (about 5%) and their high charge to mass ratio, ie, their fast ... Cited by 3
L Yin, BJ Albright, D Jung, KJ Bowers, RC Shah… - Physics of …, 2011 - link.aip.org ... Simulations show that relativistic transparency occurs before significant ion energies are attained in a prior accelerationphase possibly dominated by RPA and that the bulk of the ion acceleration occurs during transparency. ... Cited by 2 - Related articles - All 3 versions
BM Bein, S Berkebile-Stoiser… - The Astrophysical …, 2011 - iopscience.iop.org ... After the main impulsive accelerationphase the CME propagates at almost constant velocity or shows a gradual acceleration/deceleration due to interaction with the ambient solar wind flow during propagation in the interplanetary space (eg, Gopalswamy et al. 2000). ...
AD Joshi… - The Astrophysical Journal, 2011 - iopscience.iop.org ... Zhang & Dere (2006), the initiation phase is the phase of slow rise of CMEs; in the acceleration phase they undergo a very rapid increase in their velocity; while in the propagation phase the CME velocity remains more or less constant, ie, it experiences almost zero acceleration. ...
X Jing, P Wu, F Liu, B Wu… - Aviation, Space, and …, 2011 - ingentaconnect.com ... However, in the GI group, mean HR remained stable in relation to baseline HR in the pre-accelerationphase, post-accelerationphase, and after centrifuge training, and only increased during the accelerationphase. Conversely ... All 2 versions
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