论文信息 - The radial dependence of the solar energetic particle flux - 字舞流文

The radial dependence of the solar energetic particle flux

Researchers discuss the radial dependence of the peak flux and the fluence of solar flare produced energetic particles under the assumption that they propagate diffusively in the heliosphere.

[1] D. Hamilton,et al. A multispacecraft study of the injection and transport of solar energetic particles , 1987 .

[2] H. Kunow,et al. Interplanetary pitch angle scattering and coronal transport of solar energetic particles: New information from Helios , 1980 .

[3] D. Hamilton. The radial transport of energetic solar flare particles from 1 to 6 AU , 1977 .

[4] C. Ng,et al. Propagation of solar-flare cosmic rays along corotating interplanetary flux-tubes , 1975 .

[5] J. Quenby,et al. A comparison of theoretical and experimental estimates of the solar proton diffusion coefficient during three flare events , 1973 .

[6] J. Lupton,et al. Solar flare particle propagation: Comparison of a new analytic solution with spacecraft measurements , 1973 .

[7] D. Hamilton. Dynamics of solar cosmic ray events: Processes at large heliocentric distances (⪢1 AU)☆ , 1981 .

[8] W. Webber,et al. Solar Proton Propagation Characteristics Out to 16 AU , 1979 .

[9] Eugene N. Parker,et al. THE PASSAGE OF ENERGETIC CHARGED PARTICLES THROUGH INTERPLANETARY SPACE , 1965 .

[10] R. E. Marshak,et al. Interplanetary Dynamical Processes , 1963 .