Zobrazeno 1 - 10
of 78
pro vyhledávání: '"Jones, Frank C."'
Publikováno v:
Astrophys.J.600:485-500,2004
Shock jump conditions are obtained for steady-state, plane shocks with oblique magnetic fields and arbitrary flow speeds. For ultrarelativistic and nonrelativistic shocks, the jump conditions may be solved analytically. For mildly relativistic shocks
Externí odkaz:
http://arxiv.org/abs/astro-ph/0307428
In an attempt to understand the source and propagation of galactic cosmic rays we have employed the Modified Weighted Slab technique along with recent values of the relevant cross sections to compute primary to secondary ratios including B/C and Sub-
Externí odkaz:
http://arxiv.org/abs/astro-ph/0007293
We have modeled the injection and acceleration of pickup ions at the solar wind termination shock and investigated the parameters needed to produce the observed Anomalous Cosmic Ray (ACR) fluxes. A non-linear Monte Carlo technique was employed which
Externí odkaz:
http://arxiv.org/abs/astro-ph/9910126
There has recently been interest in the role of inverse bremsstrahlung, the emission of photons by fast suprathermal ions in collisions with ambient electrons possessing relatively low velocities, in tenuous plasmas in various astrophysical contexts.
Externí odkaz:
http://arxiv.org/abs/astro-ph/9908327
We have modeled the injection and acceleration of pickup ions at the solar wind termination shock and investigated the parameters needed to produce the observed Anomalous Cosmic Ray (ACR) fluxes. A non-linear Monte Carlo technique was employed, which
Externí odkaz:
http://arxiv.org/abs/astro-ph/9809137
We give a rigorous derivation of a theorem showing that charged particles in an arbitrary electromagnetic field with at least one ignorable spatial coordinate remain forever tied to a given magnetic-field line. Such a situation contrasts the signific
Externí odkaz:
http://arxiv.org/abs/astro-ph/9808103
We have developed a Monte Carlo technique for self-consistently calculating the hydrodynamic structure of oblique, steady-state shocks, together with the first-order Fermi acceleration process and associated non-thermal particle distributions. This i
Externí odkaz:
http://arxiv.org/abs/astro-ph/9609182
Publikováno v:
American Scientist, 1973 Sep 01. 61(5), 518-521.
Externí odkaz:
https://www.jstor.org/stable/27843978
