Reconstruction of Helio-Latitudinal Structure of the Solar Wind Proton Speed and Density
Reconstruction of Helio-Latitudinal Structure of the Solar Wind Proton Speed and Density
The modeling of the heliosphere requires continuous three-dimensional solar wind data. The in-situ out-of-ecliptic measurements are very rare, so that other methods of solar wind detection are needed. We use the remote-sensing data of the solar wind speed from observations of interplanetary scintillation (IPS) to reconstruct spatial and temporal structures …