Search Results - "Bzowski, M"
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WawHelioIonMP: A Semiempirical Tool for the Determination of Latitudinal Variation in the Ionization Rate of Interstellar Hydrogen and the Solar Wind
Published in The Astrophysical journal (01-05-2024)“…Abstract The latitudinal structure of the solar wind varies during the cycle of solar activity. Analysis of this variation is important for understanding the…”
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A New 3D Solar Wind Speed and Density Model Based on Interplanetary Scintillation
Published in The Astrophysical journal. Supplement series (01-03-2022)“…Abstract The solar wind (SW) is an outflow of the solar coronal plasma, which expands supersonically throughout the heliosphere. SW particles interact by…”
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On the General Correlation between 3D Solar Wind Speed and Density Model and Solar Proxies
Published in The Astrophysical journal. Supplement series (01-01-2023)“…Abstract 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…”
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Time Delay between Outer Heliosheath Crossing and Observation of Interstellar Neutral Atoms
Published in The Astrophysical journal (01-09-2020)“…In situ measurements of the heliospheric particle populations by the Voyager spacecraft can only be put in an appropriate context with remote-sensing…”
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Sun-Heliosphere Observation-based Ionization Rates Model
Published in The Astrophysical journal (01-07-2020)“…The solar wind (SW) and the extreme ultraviolet (EUV) radiation modulate fluxes of interstellar and heliospheric particles inside the heliosphere both in time…”
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Effects of Heliolatitudinal Anisotropy of Solar Far-ultraviolet/Extreme-ultraviolet Emissions on Lyα Helioglow
Published in The Astrophysical journal (01-02-2024)“…Abstract We present a study of the influence of solar UV anisotropy on the heliospheric backscatter helioglow generated by resonant scattering of solar Ly α…”
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On the Sensitivity of Heliosphere Models to the Uncertainty of the Low-energy Charge Exchange Cross-section
Published in The Astrophysical journal (01-01-2020)“…Models play an important role in our understanding of the global structure of the solar wind and its interaction with the interstellar medium. A critical…”
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The Heliosphere Is Not Round
Published in The Astrophysical journal (20-07-2018)“…Observations from the Ion and Neutral Camera (INCA) on the Cassini mission of energetic neutral atoms (ENAs) at ∼10 keV and ∼45 keV showed significant…”
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Radiation Pressure Acting on the Neutral He Atoms in the Heliosphere
Published in The Astrophysical journal (01-06-2023)“…Abstract Interstellar neutral helium (ISN He) is an important source of information on the physical state of the local interstellar medium. Radiation pressure…”
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Sensitivity of the Helioglow to Variation of the Total Ionization Rate and Solar Lyα Emission
Published in The Astrophysical journal (01-04-2024)“…Abstract Direct observations of solar wind are mostly limited to the vicinity of the ecliptic plane. Retrieving the latitudinal structure of solar wind…”
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Determining the Ionization Rates of Interstellar Neutral Species Using Direct-sampling Observations of Their Direct and Indirect Beams
Published in The Astrophysical journal. Supplement series (01-03-2023)“…Abstract A good understanding of the ionization rates of neutral species in the heliosphere is important for studies of the heliosphere and planetary…”
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Science Opportunities for IMAP-Lo Observations of Interstellar Neutral Hydrogen and Deuterium during a Maximum of Solar Activity
Published in The Astrophysical journal. Supplement series (01-04-2024)“…Abstract Direct-sampling observations of interstellar neutral gas, including hydrogen and deuterium, have been performed for more than one cycle of solar…”
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The Direction of the Flow of Interstellar Neutral H Based on Photometric Observations from SOHO/SWAN
Published in The Astrophysical journal (01-07-2023)“…Abstract Interstellar neutral hydrogen flows into the heliosphere as a mixture of the primary and secondary populations from two somewhat different directions…”
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Energetic Neutral Atoms from the Heliosheath as an Additional Population of Neutral Hydrogen in the Inner Heliosphere
Published in The Astrophysical journal (10-01-2019)“…Interstellar neutral hydrogen (ISN H) gas penetrates freely the heliopause. Inside the inner heliosheath, the charge-exchange interaction of this gas with the…”
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Absorption of the Lyα Radiation in the Heliosphere
Published in The Astrophysical journal (01-02-2022)“…Abstract Absorption of the Ly α radiation on interstellar neutral hydrogen (ISN H) atoms in the heliosphere is a potentially important effect to account for in…”
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Interstellar Conditions Deduced from Interstellar Neutral Helium Observed by IBEX and Global Heliosphere Modeling
Published in The Astrophysical journal (01-08-2023)“…Abstract In situ observations of interstellar neutral (ISN) helium atoms by the IBEX-Lo instrument on board the Interstellar Boundary Explorer (IBEX) mission…”
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Science Opportunities for IMAP-Lo Observations of Interstellar Neutral Helium, Neon, and Oxygen during a Maximum of Solar Activity
Published in The Astrophysical journal. Supplement series (01-11-2023)“…Abstract Direct-sampling observations of interstellar neutral (ISN) species and their secondary populations give information about the physical state of the…”
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Relative In-flight Response of IBEX-Lo to Interstellar Neutral Helium Atoms
Published in The Astrophysical journal. Supplement series (01-05-2023)“…Abstract The IBEX-Lo instrument on the Interstellar Boundary Explorer (IBEX) mission measures interstellar neutral (ISN) helium atoms. The detection of helium…”
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Very Local Interstellar Medium Revealed by a Complete Solar Cycle of Interstellar Neutral Helium Observations with IBEX
Published in The Astrophysical journal. Supplement series (01-04-2022)“…Abstract The IBEX-Lo instrument on board the Interstellar Boundary Explorer (IBEX) mission samples interstellar neutral (ISN) helium atoms penetrating the…”
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Breaking Correlation in the Inflow Parameters of Interstellar Neutral Gas in Direct-sampling Observations
Published in The Astrophysical journal (01-10-2022)“…Abstract We analyze the reasons for the correlation between the temperature, direction, and speed of the interstellar neutral gas inflow into the heliosphere,…”
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