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Kinetic Properties of Coronal Gas
Hydrostatic Properties of a Coronal Atmosphere
11 other sections not shown
adiabatic approximation Astrophys asymptotic atmosphere Bernoulli equation blast wave boundary cm2/sec consider convection coronal expansion coronal heating coronal temperature cosmic ray intensity critical point discussed in Chapter disordered disordered field drift effects electron enhanced corona expanding corona flow follows Forbush decrease galactic cosmic ray gauss geomagnetic storm gives gradient hydrodynamic increases infinity inner solar system instability interplanetary fields interplanetary magnetic field interplanetary space interstellar interstellar medium ions km/sec large-scale lines of force lower branch magnetic tongue main sequence mean free path motion observed orbit of Earth outward Parker particle density Phys plasma polytrope pressure protons quiet-day solar wind radial distance radius readily shown reference level region result scale scattering centers shell shock transition Simpson solar activity solar corona solar corpuscular radiation solar flare solar particles solar wind velocity solution spectrum stars stationary stellar wind streamers thermal conduction tion zero