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Scattering of Continuously Injected Pickup Ions of Oblique Pickup Angles in the Outer Heliosheath
Pitch angle scattering of pickup ions (PUIs) in the outer heliosheath is studied using two-dimensional hybrid simulations, with the PUIs continuously injected at specified injection rates and pickup angles.
Ding Sheng +3 more
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X-ray scattering by interstellar dust.
This thesis reports work carried out to make a first observation of x-rays scattered by interstellar dust grains. Initially, important data about the dust, obtained at wavelengths ranging from the infra-red to ultra-violet spectral regions, are discussed
Daniel. Rolf (7659299)
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Scattering of Pulsar Radiation in the Interstellar Medium [PDF]
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Note: Rayleigh Scattering in Interstellar Space
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ScatteringOptics.jl: An Interstellar Scattering Framework in the Julia Programming Language
Anna Tartaglia +2 more
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Interstellar scattering as a cosmological probe
Since the discovery that the flux densities of very compact astrophysical sources are modulated by scattering in the inhomogeneous, ionized interstellar medium (ISM) of our own Galaxy through a phenomenon known as Interstellar Scintillation (ISS), these ...
Hayley Bignall +2 more
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Interstellar scattering of SgrA∗
AIP Conference Proceedings, 1988SgrA* is a compact, nonthermal radio source located in the center of the dense stellar cluster that defines the center of our galaxy. The effects of interstellar propagation, or limits thereon, on signals form SgrA* will be described.
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Some Scattering Problems of Interstellar Grains [PDF]
Some general effects of size, shape, and material on the scattering properties of small particles are considered with a view to determining their relative importance to interstellar dust interpreatations.
J Mayo Greenberg
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Anisotropy in Pulsar Interstellar Scattering
Chinese Journal of Astronomy and Astrophysics, 2006Pulsar observers have to contend with several effects of propagation through the ionized interstellar medium. I review those effects and how they can be used to study the interstellar plasma. Pulsars are normally observed under conditions of strong scintillation and show both diffractive and refractive effects. I emphasize the diffractive scintillation
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