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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 Hot Interstellar Medium
The interstellar medium (ISM) of galaxies very often contains a gas component that reaches the temperature of several million degrees, whose physical...
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Infrared Spectroscopy of H+3 in the Interstellar Medium
Long a subject of laboratory and theoretical studies, H+3indexAH+3 is now recognized to be a fundamental ingredient of interstellar space, as the...
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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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A possible direct exposure of the Earth to the cold dense interstellar medium 2–3 Myr ago
Cold, dense clouds in the interstellar medium of our Galaxy are 4–5 orders of magnitude denser than their diffuse counterparts. Our Solar System has...
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Low-energy cosmic rays: regulators of the dense interstellar medium
Low-energy cosmic rays (up to the GeV energy domain) play a crucial role in the physics and chemistry of the densest phase of the interstellar...
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Simulation study of optical turbulence in interstellar medium by phase screens
The interstellar medium (ISM) is the most widely interested in astronomical fields. Understanding the behavior of the interstellar medium is needed...
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Radioactive isotopes in the interstellar medium
Radioactive components of the interstellar medium provide an entirely-different and new aspect to the studies of the interstellar medium. Injected...
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Observations of the Outer Heliosphere, Heliosheath, and Interstellar Medium
The Voyager spacecraft have left the heliosphere and entered the interstellar medium, making the first observations of the termination shock,...
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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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Shocks in the Very Local Interstellar Medium
Large-scale disturbances generated by the Sun’s dynamics first propagate through the heliosphere, influence the heliosphere’s outer boundaries, and...
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Propagation of shock waves in a non-ideal gas with dust particles in an interstellar medium
The present paper demonstrates the study of propagation of converging shock waves in a spherical interstellar cloud of an non-ideal gas (van der...
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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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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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Interaction of the Supersonic Stellar Wind with Free Stream of the Interstellar Medium: the Effect of the Azimuthal Magnetic Field of the Star
AbstractThe problem of the interaction of a hypersonic stellar wind with the surrounding interstellar medium is considered. The media are assumed to...
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The Hot Interstellar Medium
The interstellar medium (ISM) of galaxies very often contains a gas component that reaches the temperature of several million degrees, whose physical...
