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A new 3D solar wind speed and density model based on interplanetary scintillation
C. Porowski, M. Bzowski, M. Tokumaru
The solar wind (SW) is an outflow of the solar coronal plasma, expanding supersonically throughout the heliosphere. SW particles interact by charge exchange with interstellar neutr…
Influence of Heliolatitudinal Anisotropy of Solar FUV/EUV Emissions on Lyman-alpha Helioglow: SOHO/SWAN Observations and WawHelioGlow Modeling
Marek Strumik, Maciej Bzowski, Marzena A. Kubiak
Observations of the Sun's surface suggest a nonuniform radiated flux as related to the presence of bright active regions and darker coronal holes. The variations of the FUV/EUV sou…
WawHelioGlow: a model of the heliospheric backscatter glow. II. The helioglow buildup and the potential significance of the anisotropy in the solar EUV output
M. A. Kubiak, M. Bzowski, I. Kowalska-Leszczynska +1
The helioglow is a fluorescence of interstellar atoms inside the heliosphere, where they are excited by the solar EUV. Because the mean free path between collisions for the interst…
WawHelioGlow: a model of the heliospheric backscatter glow. I. Model definition
M. A. Kubiak, M. Bzowski, I. Kowalska-Leszczynska +1
The helioglow is a fluorescence of interstellar atoms inside the heliosphere, where they are excited by the solar EUV emission. So far, the helioglow of interstellar H and He have…