output
20022009
most citedDirect observation of Anderson localization of matter-waves in a controlled disorder

1.6k citations

Showing 2006 · astro-phShow all

18 papers · 2 filters

astro-ph200682 cited

The evolution of clusters in the CLEF cosmological simulation: X-ray structural and scaling properties

Scott T. Kay, Antonio C. da Silva, Nabila Aghanim +5

We present results from a study of the X-ray cluster population that forms within the CLEF cosmological hydrodynamics simulation, a large N-body/SPH simulation of the Lambda CDM co…

astro-ph200613 cited

High resolution gamma ray spectroscopy of flares on the east and west limbs of the Sun

M. J. Harris, V. Tatischeff, J. Kiener +2

A new generation of Ge-based high-resolution gamma-ray spectrometers has allowed accurate measurements to be made of the profiles, widths and energies of the gamma-ray lines emitte…

astro-ph200640 cited

Identification of backgrounds in the EDELWEISS-I dark matter search experiment

S. Fiorucci, A. Benoit, L. Berge +36

This paper presents our interpretation and understanding of the different backgrounds in the EDELWEISS-I data sets. We analyze in detail the several populations observed, which inc…

astro-ph2006125 cited

Multi-scale Hall-MHD turbulence in the solar wind

S. Galtier, E. Buchlin

Solar wind magnetic fluctuation spectra exhibit a significant power law steepening at frequencies f>1Hz. The origin of this multi-scaling is investigated through dispersive Hall ma…

astro-ph200634 cited

Is 6-Li in metal-poor halo stars produced in situ by solar-like flares?

V. Tatischeff, J. -P. Thibaud

The high 6-Li abundances recently measured in metal-poor halo stars are far above the value predicted by Big Bang nucleosynthesis. They cannot be explained by galactic cosmic-ray i…

astro-ph20062 cited

Plasma diagnostic of a solar prominence from hydrogen and helium resonance lines

N. Labrosse, J. -C. Vial, P. Gouttebroze

We present the first comparison of profiles of H et He resonance lines observed by SUMER with theoretical profiles computed with our non-LTE radiative transfer code. We use the H I…