32 citations · 62 across the 7 of their papers we have counts for
12 papers
Interstellar Neutral Hydrogen in the Heliosphere: New Horizons Observations in the Context of Models
P. Swaczyna, M. Bzowski, K. Dialynas +12
Interstellar neutral (ISN) hydrogen is the most abundant species in the outer heliosheath and the very local interstellar medium (VLISM). Charge exchange collisions in the outer he…
Sensitivity of the helioglow to variation of the total ionization rate and solar Lyman-alpha emission
Izabela Kowalska-Leszczynska, Marzena A. Kubiak, Maciej Bzowski +1
Direct observations of solar wind are mostly limited to the vicinity of the ecliptic plane. Retrieving the latitudinal structure of solar wind indirectly based on observations of t…
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…
Radiation pressure acting on the neutral He atoms in the Heliosphere
Izabela Kowalska-Leszczynska, Marzena A. Kubiak, Maciej Bzowski
The Interstellar Neutral Helium (ISN He) is an important source of information on the physical state of the Local Interstellar Medium. Radiation pressure acting on the neutral heli…
Absorption of the Lyman- radiation in the heliosphere
Izabela Kowalska-Leszczynska, Marzena A. Kubiak, Maciej Bzowski
Absorption of the Lyman- radiation on Interstellar Neutral Hydrogen (ISN H) atoms in the heliosphere is a potentially important effect to account for in precise gas distribution…
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…