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On the General Correlation between 3D Solar Wind Speed and Density Model and Solar Proxies

Bzowski, M.; Tokumaru, M.; Porowski, C.

The solar wind (SW) is a supersonic outflow of plasma from the solar corona, with the latitudinal speed and density profiles varying with the solar activity. The SW protons charge exchange with the inflowing interstellar neutral atoms and create energetic neutral atoms (ENAs), which bring information on the physical state of the plasma within the …