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Pioneer-10 observation of the solar wind proton temperature heliocentric gradient

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Abstract

Solar wind isotropic proton temperatures as measured out to 12.2 AU heliocentric distance by the Ames plasma analyzer aboard Pioneer-10 are presented as consecutive averages over three Carrington solar rotations and discussed. The weighted least-squares fit of average temperature to heliocentric radial distance, R, yields the power law R -0.52. These average proton temperatures are not correlated as well with Pioneer-10's heliocentric radial distance (-0.85) as are the corresponding average Zürich sunspot numbers R z (-0.95). Consequently, it is difficult to isolate the spatial gradient in the Pioneer-10 solar wind proton temperatures using that data alone.

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Mihalov, J.D., Wolfe, J.H. Pioneer-10 observation of the solar wind proton temperature heliocentric gradient. Sol Phys 60, 399–406 (1978). https://doi.org/10.1007/BF00156539

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  • DOI: https://doi.org/10.1007/BF00156539

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