We analyse the temperature anisotropy of the protons in the solar wind and thereby concentrate on plasma data obtained in the year 1976 of the Helios 1 and Helios 2 missions. We derive the core proton temperatures and . in the directions perpendicular and parallel to the magnetic field. as well as the core parallel plasma beta. https://www.bekindtopets.com/mega-offer-Shot-AI-Cyberpunk-Steel-Tip-Darts-25gm-super-offer/
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