activity
20122020
most citedInterstellar Pickup Ion Observations to 38 AU

85 citations · 524 across the 15 of their papers we have counts for

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Showing astro-ph.SRShow all

11 papers · 1 filter

astro-ph.SR2020★ 30 cited

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…

astro-ph.SR2019★ 19 cited

Science Opportunities from Observations of the Interstellar Neutral Gas with Adjustable Boresight Direction

Justyna M. Sokół, Marzena A. Kubiak, Maciej Bzowski +2

The interstellar neutral (ISN) gas enters the heliosphere and is detected at a few au from the Sun, as demonstrated by Ulysses and the nterstellar Boundary Explorer (IBEX) missions…

astro-ph.SR2019★ 11 cited

Heliospheric structure as revealed by the 3 -- 88 keV H ENA spectra

A. Czechowski, M. Bzowski, J. M. Sokół +8

Energetic neutral atoms (ENA) are an important tool for investigating the structure of the heliosphere. Recently, it was observed that fluxes of ENAs (with energy 55 keV) com…

astro-ph.SR2019★ 56 cited

Interstellar neutral helium in the heliosphere from IBEX observations. VI. The He density and the ionization state in the Very Local Interstellar Matter

M. Bzowski, A. Czechowski, P. C. Frisch +14

Interstellar neutral gas atoms penetrate the heliopause and reach 1~au, where they are detected by IBEX. The flow of neutral interstellar helium through the perturbed interstellar…

astro-ph.SR2019★ 36 cited

Interstellar Neutral Gas Species And Their Pickup Ions Inside The Heliospheric Termination Shock. The Large-scale Structures

Justyna M. Sokół, Marzena A. Kubiak, Maciej Bzowski

We study the distribution of the interstellar neutral (ISN) gas density and the pick-up ion (PUI) density of hydrogen, helium, neon, and oxygen in the heliosphere for heliocentric…

astro-ph.SR2018★ 33 cited

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…

astro-ph.SR2018★ 38 cited

Interstellar neutral helium in the heliosphere from IBEX observations. V. Observations in IBEX-Lo ESA steps 1, 2, & 3

Paweł Swaczyna, Maciej Bzowski, Marzena A. Kubiak +9

Direct-sampling observations of interstellar neutral (ISN) He by Interstellar Boundary Explorer (IBEX) provide valuable insight into the physical state of and processes operating i…

astro-ph.SR2017★ 41 cited

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…

astro-ph.SR2016★ 27 cited

Solar cycle variation of interstellar neutral He, Ne, O density and pick-up ions along the Earth's orbit

Justyna M. Sokół, Maciej Bzowski, Marzena A. Kubiak +1

We simulated the modulation of the interstellar neutral (ISN) He, Ne, and O density and pick-up ion (PUI) production rate and count rate along the Earth's orbit over the solar cycl…

astro-ph.SR2016★ 30 cited

The energy-dependent position of the IBEX ribbon due to the solar wind structure

Paweł Swaczyna, Maciej Bzowski, Justyna M. Sokół

Observations of energetic neutral atoms (ENAs) allow for remote studies of the plasma condition in the heliosphere and the neighboring local interstellar medium. The first IBEX res…

astro-ph.SR2014★ 6 cited

Photoionization rates for helium: update

Justyna M. Sokół, Maciej Bzowski

The NIS He gas has been observed at a few AU to the Sun almost from the beginning of the space age. To model its flow an estimate of the loss rates due to ionization by solar extre…