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.diegojavierfares.com/flash-pick-Hasport-Billet-Rear-K-swap-Mount-92-95-Civic-94-01-Integra-great-buy/