Ion Abundances in the Solar Wind |
Common terms and phrases
abundances amounts Appendix approximation assumed atoms azimuthal Bame calculations charge exchange collisions compared cross-sections dependence determine direction discussed Ecliptic Plane effect electron elements energy equation example expansion experimental expression Figure flow Function further given He++ HELIOCENTRIC DISTANCE helium Hence Hundhausen hydrogen hydrogen atoms increases indicate Indirect infall initial injected integral interaction interstellar medium involves ionization ionization structure ions iron km/sec less limit Lyman alpha magnetic field measurements nearly neutral neutral hydrogen observations occur oxygen peak percent photo-ionization possible present probability processes produce proton radiation range ratio reaction reaction rate recombination references region relative reported respectively satellite scale separation shown solar corona solar cosmic rays solar wind solar wind plasma space spectra suggested symmetric Table temperature thermal trajectories unit values various vary Vela velocity distribution