On the He(2+) to H(+) temperature ratio in slow solar wind

Details On the He(2+) to H(+) temperature ratio in slow solar wind On the He(2+) to H(+) temperature ratio in slow solar wind

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987jgr....92.7723h&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 92, July 1, 1987, p. 7723-7727.

Physics

7

Coulomb Collisions, Helium Ions, Hydrogen Ions, Plasma Temperature, Solar Wind Velocity, Helios Project, Particle Energy, Proton Energy

Scientific paper

On the basis of a three-fluid model with energy exchange by Coulomb collisions and heat flux degradation the ratio T of alpha to proton temperatures is investigated. For various relative ion densities and plasma parameters the collisional evolution of T is modeled and compared with Helios in situ measurements. Good agreement between data and theory is found.

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