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The flow direction of interstellar neutral H from SOHO/SWAN
M. Bzowski, M. A. Kubiak, M. Strumik +3
Interstellar neutral hydrogen flows into the heliosphere as a mixture of the primary and secondary populations from two somewhat different directions due to splitting occurring in…
Determining the ionization rates of interstellar neutral species using direct-sampling observations of their direct and indirect beams
M. Bzowski, M. A. Kubiak, E. Moebius +1
A good understanding of the ionization rates of neutral species in the heliosphere is important for studies of the heliosphere and planetary atmospheres. So far, the intensities of…
On general correlation between 3D solar wind speed and density model and solar proxies
C. Porowski, M. Bzowski, M. Tokumaru
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…
Breaking correlation in the inflow parameters of interstellar neutral gas in direct-sampling observations
M. Bzowski, M. A. Kubiak, E. Möbius +1
We analyze the reasons for the correlation between the temperature, direction, and speed of the interstellar neutral gas inflow into the heliosphere, obtained in analyzes of observ…
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…