Solar Cosmic Rays, Том 2National Aeronautics and Space Administration and the National Science Foundation, Washington, D.C., 1976 - Всего страниц: 1164 |
Содержание
SOLAR COSMIC RAYS AS A SOURCE | 1 |
Methods of Studying Solar Cosmic Rays | 8 |
Sensitivity of Solar Particles to Physical Conditions | 27 |
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absorption acceleration according alloy anisotropy approximation beam chromospheric chromospheric flares components composite crystals curves decrease deformation density dependence determined diameter diffusion coefficient distribution Earth effect elastic electrons emission energy equation eutectic experimental fibers Figure filters flux Forbush effects function galactic galactic cosmic rays geomagnetic geomagnetic storm Geophys increase intensity interplanetary magnetic field interplanetary space ionosphere irregularities July kg/mm² lines of force longitudinal low-energy magnetic field matrix maximum measurements mechanism medium metal method modulus mullite neutrons November November 12 nuclei observed obtained outburst parameters plasma plastics polar polymer porosity possible production propagation properties radiation range ratio region reinforced material rigidity satellite September shear shown sintering solar activity solar cosmic rays solar flares solar particles solar protons spectra spectrum of solar strength stresses structure studied temperature tensile thermal transverse tungsten velocity waves whiskers
