activity
19982018
most citedDust in the Local Interstellar Wind

220 citations · 2.8k across the 77 of their papers we have counts for

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Showing 2012Show all

12 papers · 1 filter

physics.plasm-ph2012★ 12 cited

String structures in driven 3D complex plasma clusters

L. Wörner, C. Räth, V. Nosenko +5

The structure of driven three-dimensional complex plasma clusters was studied experimentally. The clusters consisted of around 60 hollow glass spheres with a diameter of 22 microns…

physics.plasm-ph2012★ 19 cited

Three-dimensional structure of Mach cones in monolayer complex plasma

L. Couedel, D. Samsonov, C. Durniak +4

Structure of Mach cones in a crystalline complex plasma has been studied experimentally using an intensity sensitive imaging, which resolved particle motion in three dimensions. Th…

astro-ph.CO2012★ 23 cited

Scale dependent non-Gaussianities in the CMB data identified with Minkowski Functionals and Scaling Indices

H. I. Modest, C. Räth, A. J. Banday +6

In order to test for non-Gaussianities with respect to scale-dependencies we use so-called surrogate maps, in which possible phase correlations of the Fourier phases of the origina…

physics.plasm-ph2012★ 21 cited

Nonviscous motion of a slow particle in the dust crystal under microgravity conditions

D. I. Zhukhovitskii, V. E. Fortov, V. I. Molotkov +6

Subsonic motion of a large particle moving through the bulk of a dust crystal formed by negatively charged small particles is investigated using the PK-3 Plus laboratory onboard th…

astro-ph.CO2012★ 8 cited

Probing non-Gaussianities in the CMB on an incomplete sky using surrogates

G. Rossmanith, H. Modest, C. Räth +3

We demonstrate the feasibility to generate surrogates by Fourier-based methods for an incomplete data set. This is performed for the case of a CMB analysis, where astrophysical for…

physics.plasm-ph2012★ 23 cited

Interaction of two-dimensional plasma crystals with upstream charged particles

C. -R. Du, V. Nosenko, S. Zhdanov +2

Two-dimensional plasma crystals are characterized by a strong up-and-down asymmetry not only due to gravity but also due to the presence of plasma flow at the location of particles…