Solar cycle invariance in solar wind proton temperature relationships

Details Solar cycle invariance in solar wind proton temperature relationships Solar cycle invariance in solar wind proton temperature relationships

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987jgr....9211189l&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 92, Oct. 1, 1987, p. 11189-11194. NASA-supported research.

Physics

68

Proton Energy, Solar Cycles, Solar Protons, Solar Wind Velocity, Data Reduction, Magnetohydrodynamic Waves, Solar Flux, Velocity Measurement

Scientific paper

The relationships between solar wind proton temperature and velocity and between temperature and momentum flux density at 1 AU are examined using National Space Science Data Center IMP 8 solar wind data obtained from late 1984 to early 1985. These relationships are compared with similar ones obtained from a variety of solar wind data spanning 14 years, from 1966 to 1980. It is found that these relationships, particularly the one between temperature and velocity, are very stable over the solar cycles from which these data were drawn. This suggests that the basic physical processes which accelerate and heat the solar wind have remained unchanged for the last 20 years.

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