Computer modeling of test particle acceleration at oblique shocks
暂无分享,去创建一个
[1] I. N. Toptyghin. Acceleration of particles by shocks in a cosmic plasma , 1980 .
[2] H. Helfer. Magneto-Hydrodynamic Shock Waves. , 1953 .
[3] M. Pesses. On the conservation of the first adiabatic invariant in perpendicular shocks. [in space plasmas] , 1981 .
[4] Derek A. Tidman,et al. Shock waves in collisionless plasmas , 1971 .
[5] J. Sakai,et al. Particle acceleration by magnetic reconnection and shocks during current loop coalescence in solar flares , 1988 .
[6] S. Krimigis,et al. Shock-associated low-energy ion enhancements observed by Voyagers 1 and 2 , 1981 .
[7] M. Dryer,et al. Pioneer 9 and Ogo 5 observations of an interplanetary multiple shock ensemble on February 2, 1969 , 1975 .
[8] Z. Němeček,et al. Acceleration of electrons at the quasi-perpendicular bow shock according to intershock data , 1986 .
[9] A. Owens. An algorithm for generating fluctuations having any arbitrary power spectrum , 1978 .
[10] J. Jokipii. Rate of energy gain and maximum energy in diffusive shock acceleration , 1987 .
[11] C. Cesarsky,et al. The maximum energy of cosmic rays accelerated by supernova shocks , 1983 .
[12] T. Terasawa. Energy spectrum and pitch angle distribution of particles reflected by MHD shock waves of fast mode , 1979 .
[13] J. Jokipii. Particle drift, diffusion, and acceleration at shocks , 1982 .
[14] J. Bendat,et al. Random Data: Analysis and Measurement Procedures , 1971 .
[15] C. Russell,et al. Plasma and energetic particle structure upstream of a quasi-parallel interplanetary shock , 1984 .
[16] R. Decker. The modulation of low‐energy proton distributions by propagating interplanetary shock waves: A numerical simulation , 1981 .
[17] C. Kennel,et al. Plasma rest frame distributions of suprathermal ions in the earth's foreshock region , 1981 .
[18] L. Vlahos,et al. Shock drift acceleration in the presence of waves , 1985 .
[19] D. Winske,et al. HYBRID SIMULATION CODES WITH APPLICATION TO SHOCKS AND UPSTREAM WAVES , 1985 .
[20] William H. Matthaeus,et al. Measurement of the rugged invariants of magnetohydrodynamic turbulence in the solar wind , 1982 .
[21] A. Brinca. On the coupling of test ions to magnetoplasma flows through turbulence , 1984 .
[22] L. Burlaga. MHD processes in the outer heliosphere , 1984 .
[23] E. Sarris,et al. Dominant acceleration processes of ambient energetic protons (E ⩾ 50 keV) at the Bow Shock: Conditions and limitations , 1983 .
[24] C. Russell,et al. Upstream hydromagnetic waves and their association with backstreaming ion populations: ISEE 1 and 2 observations , 1981 .
[25] D. Winske,et al. Diffuse ions produced by electromagnetic ion beam instabilities. [in earth's bow shock , 1984 .
[26] S. Krimigis,et al. Quasi-perpendicular shock acceleration of ions to about 200 MeV and electrons to about 2 MeV observed by Voyager 2 , 1985 .
[27] P. C. Hedgecock. Measurements of the interplanetary magnetic field in relation to the modulation of cosmic rays , 1975 .
[28] C. Russell,et al. Upstream waves and particles , 1983 .
[29] J. Earl. The diffusive idealization of charged-particle transport in random magnetic fields. [cosmic ray propagation] , 1974 .
[30] Y. Ohsawa. Resonant Ion Acceleration by Oblique Magnetosonic Shock Wave in a Collisionless Plasma , 1985 .
[31] C. Wu. A fast Fermi process: Energetic electrons accelerated by a nearly perpendicular bow shock , 1984 .
[32] D. Burgess. Shock drift acceleration at low energies , 1987 .
[33] Y. Ohsawa. ACCELERATION OF ENERGETIC IONS BY A NEARLY PERPENDICULAR INTERPLANETARY SHOCK , 1986 .
[34] B. Sonnerup. Acceleration of particles reflected at a shock front , 1969 .
[35] D. Potter. Acceleration of electrons by interplanetary shocks , 1981 .
[36] H. A. Luther,et al. Applied numerical methods , 1969 .
[37] T. Sanderson,et al. The energy spectrum of 35‐ to 1600‐keV protons associated with interplanetary shocks , 1984 .
[38] D. Eichler. Energetic particle spectra in finite shocks: the earth's bow shock , 1981 .
[39] J. Sakai,et al. Non-stochastic prompt proton acceleration by fast magnetosonic shocks in the solar plasma , 1986 .
[40] L. Vlahos,et al. Numerical Studies of Particle Acceleration at Turbulent, Oblique Shocks with an Application to Prompt Ion Acceleration during Solar Flares , 1986 .
[41] J. F. Mckenzie,et al. Transmission of Alfvén waves through the earth's bow shock , 1969 .
[42] C. Goodrich,et al. The interaction of quasiperpendicular shock waves in a collisionless plasma , 1987 .
[43] Charles C. Goodrich,et al. The structure of perpendicular bow shocks , 1982 .
[44] D. Wentzel. Cosmic-Ray Propagation in the Galaxy: Collective Effects , 1974 .
[45] R. Decker. Formation of shock‐spike events at quasi‐perpendicular shocks , 1983 .
[46] Martin A. Lee. Coupled hydromagnetic wave excitation and ion acceleration upstream of the earth's bow shock , 1982 .
[47] S. Schwartz,et al. Ions upstream of the Earth's bow shock: A theoretical comparison of alternative source populations , 1983 .
[48] E. Greenstadt,et al. Variable field-to-normal angles in the shock foreshock boundary observed by ISEE 1 and 2 , 1985 .
[49] L. Vlahos,et al. Modeling of ion acceleration through drift and diffusion at interplanetary shocks , 1986 .
[50] W. I. Axford,et al. On the drift mechanism for energetic charged particles at shocks , 1983 .
[51] J. A. V. Allen,et al. High time resolution observations of corotating interaction region proton events by Pioneer 11 , 1984 .
[52] E. Sarris,et al. Effects of interplanetary shock waves on energetic charged particles. Progress report , 1974 .
[53] C. Kennel,et al. A parametric survey of the first critical Mach number for a fast MHD shock , 1984, Journal of Plasma Physics.
[54] L. Vlahos,et al. Predictions of lithium interactions with earth's bow shock in the presence of wave activity , 1984 .
[55] J. Gosling,et al. The electromagnetic ion beam instability upstream of the Earth's bow shock , 1981 .
[56] M. D. Montgomery,et al. Detailed directional and temporal properties of solar energetic particles associated with propagating interplanetary shock waves , 1971 .
[57] T. Armstrong,et al. The acceleration of charged particles in interplanetary shock waves , 1982 .
[58] L. Drury,et al. An introduction to the theory of diffusive shock acceleration of energetic particles in tenuous plasmas , 1983 .
[59] T. Sanderson,et al. Observations of three‐dimensional anisotropies of 35‐ to 1000‐keV protons associated with interplanetary shocks , 1985 .
[60] Y. Ohsawa. Theory for Resonant Ion Acceleration by Nonlinear Magnetosonic Fast and Slow Waves in Finite β Plasmas , 1985 .
[61] T. Northrop,et al. Adiabatic theory in regions of strong field gradients. [in magnetosphere] , 1986 .
[62] T. Chiueh. Multiple-encounter shock-drift acceleration in nearly perpendicular shocks , 1988 .
[63] S. Gary. Electromagnetic ion beam instabilities: Hot beams at interplanetary shocks , 1985 .