41 citations · 194 across the 12 of their papers we have counts for
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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…
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…
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…
Inferring contributions from unresolved point sources to diffuse emissions measured in UV sky surveys: general method and SOHO/SWAN case study
Marek Strumik, Maciej Bzowski, Izabela Kowalska-Leszczynska +1
In observations of diffuse emissions like, e.g., the Lyman- heliospheric glow, contributions to the observed signal from point sources (e.g., stars) are considered as a contamin…
Update of the Solar Lyman-Alpha Profile Line Model
Izabela Kowalska-Leszczynska, Maciej Bzowski, Marzena A. Kubiak +1
We present a modification of a model of solar cycle evolution of the solar Lyman-alpha line profile, along with a sensitivity study of interstellar neutral H hydrogen to uncertaint…
Evolution of the solar Ly- line profile during the solar cycle. II. How accurate is the present radiation pressure paradigm for interstellar neutral H in the heliosphere?
Izabela Kowalska-Leszczynska, Maciej Bzowski, Justyna M. Sokół +1
Following the derivation of a more accurate model of the evolution of the solar Lyman- line with the changing solar activity by Kowalska-leszczynska et al. 2018 (IKL18) than the…
Evolution of the Solar Lyman-Alpha line profile during the solar cycle
Izabela Kowalska-Leszczynska, Maciej Bzowski, Justyna M. Sokół +1
Recent studies of interstellar neutral (ISN) hydrogen observed by the Interstellar Boundary Explorer (IBEX) suggested that the present understanding of the radiation pressure actin…