On coronal temperatures, temperature gradients and compositions

Details On coronal temperatures, temperature gradients and compositions On coronal temperatures, temperature gradients and compositions

Mar 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...51..327n&link_type=abstract

Solar Physics, vol. 51, Mar. 1977, p. 327-343.

Physics

2

Solar Corona, Solar Electrons, Solar Temperature, Solar Wind, Electron Density (Concentration), Hydrogen Ions, Temperature Distribution, Thermal Conductivity, Wind Measurement

Scientific paper

Average solar wind properties at 1 AU either alone or together with the electron density distribution are used to obtain or review some results that relate coronal temperatures, temperature gradients, and compositions. Measured values of the temperature (T) and the temperature gradient parameter are used to find compositions that satisfy the equations used to obtain the results. The total energy equation may be satisfied if the thermal conductivity is reduced by considerable depletions of H(+) in the corona. The hydrostatic approximation (momentum equation) for the electron density distribution appears to require considerable depletions of H(+) in the corona.

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