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Future Exploration of the Outer Heliosphere and Very Local Interstellar Medium by Interstellar Probe
A detailed overview of the knowledge gaps in our understanding of the heliospheric interaction with the largely unexplored Very Local Interstellar...
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The Heliosphere and Local Interstellar Medium from Neutral Atom Observations at Energies Below 10 keV
As the heliosphere moves through the surrounding interstellar medium, a fraction of the interstellar neutral helium, hydrogen, and heavier species...
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Ultraviolet spectropolarimetry with polstar: interstellar medium science
Continuum polarization over the UV-to-microwave range is due to dichroic extinction (or emission) by asymmetric, aligned dust grains. Scattering can...
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Galactic Cosmic Rays Throughout the Heliosphere and in the Very Local Interstellar Medium
We review recent observations and modeling developments on the subject of galactic cosmic rays through the heliosphere and in the Very Local...
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Diffuse Hot Plasma in the Interstellar Medium and Galactic Outflows
We summarize observations and our current understanding of the interstellar medium (ISM) in galaxies, which mainly consists of three phases: cold...
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Comparison of the Eulerian and Lagrangian Approaches to Studying the Peculiarities of the Interstellar Dust Distribution in the Heliosphere in the Framework of the Cold Gas Model
AbstractInterstellar dust grains penetrate into the heliosphere (region in which the solar wind propagates) due to the relative motion of the Sun and...
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Size of the Solar System
The heliosphere is defined as the region of space in which the plasma and magnetic fields from the Sun are largely separate from the local...
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Periodic interstellar scintillation variations of PSRs J0613–0200 and J0636+5128 associated with the Local Bubble shell
Annual variations of interstellar scintillation can be modelled to constrain parameters of the ionized interstellar medium. If a pulsar is in a...
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Direct Exoplanet Investigation Using Interstellar Space Probes
Experience in exploring our own solar system has shown that direct investigation of planetary bodies using space probes invariably yields scientific...
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Diffuse Hot Plasma in the Interstellar Medium and Galactic Outflows
We summarize observations and our current understanding of the interstellar medium (ISM) in galaxies, which mainly consists of three phases: cold...
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Recent nucleosynthesis in the solar neighbourhood, detected with live radionuclides
In this article we try to summarize all information, gathered in the last three decades, on short-lived (order of Myr) radionuclides found in the...
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A Three-Dimensional Analytical Model of the Interstellar Extinction within the Nearest Kiloparsec
AbstractWe present a new version of our analytical model of the spatial interstellar extinction variations within the nearest kiloparsec from the...
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Gas Dynamic Models of the Interaction between the Solar Wind and Cometary Atmospheres
AbstractGas dynamic models of the interaction between the solar wind and cometary atmospheres are considered. Interest in the development of such...
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Measurements of Radioactive 60Fe and 244Pu Deposits on Earth and Moon
Earth is exposed to nearby cosmic events. The solar system moves through the interstellar medium and collects interstellar dust particles that...
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Measurements of Radioactive 60Fe and 244Pu Deposits on Earth and Moon
Earth is exposed to nearby cosmic events. The solar system moves through the interstellar medium and collects interstellar dust particles that...
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Interstellar Dust in the Solar System
Interstellar dust from the Local Interstellar Cloud was detected unambiguously for the first time in 1992 (Grün et al. in Nature 362:428–430,
1993 )....
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The Early History of Heliospheric Science and the Spacecraft That Made It Possible
Our understanding of the interaction of the large-scale heliosphere with the local interstellar medium (LISM) has undergone a profound change since...
