1,016 research outputs found
Very low sound velocities in iron-rich (Mg,Fe)O: Implications for the core-mantle boundary region
The sound velocities of (Mg_(.16)Fe_(.84))O have been measured to 121 GPa at ambient temperature using nuclear resonant inelastic x-ray scattering. The effect of electronic environment of the iron sites on the sound velocities were tracked in situ using synchrotron Mössbauer spectroscopy. We found the sound velocities of (Mg_(.16)Fe_(.84))O to be much lower than those in other presumed mantle phases at similar conditions, most notably at very high pressures. Conservative estimates of the effect of temperature and dilution on aggregate sound velocities show that only a small amount of iron-rich (Mg,Fe)O can greatly reduce the average sound velocity of an assemblage. We propose that iron-rich (Mg,Fe)O be a source of ultra-low velocity zones. Other properties of this phase, such as enhanced density and dynamic stability, strongly support the presence of iron-rich (Mg,Fe)O in localized patches above the core-mantle boundary
Anisotropy of Solar Wind Turbulence between Ion and Electron Scales
The anisotropy of turbulence in the fast solar wind, between the ion and
electron gyroscales, is directly observed using a multispacecraft analysis
technique. Second order structure functions are calculated at different angles
to the local magnetic field, for magnetic fluctuations both perpendicular and
parallel to the mean field. In both components, the structure function value at
large angles to the field S_perp is greater than at small angles S_par: in the
perpendicular component S_perp/S_par = 5 +- 1 and in the parallel component
S_perp/S_par > 3, implying spatially anisotropic fluctuations, k_perp > k_par.
The spectral index of the perpendicular component is -2.6 at large angles and
-3 at small angles, in broad agreement with critically balanced whistler and
kinetic Alfven wave predictions. For the parallel component, however, it is
shallower than -1.9, which is considerably less steep than predicted for a
kinetic Alfven wave cascade.Comment: 4 pages, 4 figures, replaced to match published versio
A Generalized Diffusion Tensor for Fully Anisotropic Diffusion of Energetic Particles in the Heliospheric Magnetic Field
The spatial diffusion of cosmic rays in turbulent magnetic fields can, in the
most general case, be fully anisotropic, i.e. one has to distinguish three
diffusion axes in a local, field-aligned frame. We reexamine the transformation
for the diffusion tensor from this local to a global frame, in which the Parker
transport equation for energetic particles is usually formulated and solved.
Particularly, we generalize the transformation formulas to allow for an
explicit choice of two principal local perpendicular diffusion axes. This
generalization includes the 'traditional' diffusion tensor in the special case
of isotropic perpendicular diffusion. For the local frame, we motivate the
choice of the Frenet-Serret trihedron which is related to the intrinsic
magnetic field geometry. We directly compare the old and the new tensor
elements for two heliospheric magnetic field configurations, namely the hybrid
Fisk and the Parker field. Subsequently, we examine the significance of the
different formulations for the diffusion tensor in a standard 3D model for the
modulation of galactic protons. For this we utilize a numerical code to
evaluate a system of stochastic differential equations equivalent to the Parker
transport equation and present the resulting modulated spectra. The computed
differential fluxes based on the new tensor formulation deviate from those
obtained with the 'traditional' one (only valid for isotropic perpendicular
diffusion) by up to 60% for energies below a few hundred MeV depending on
heliocentric distance.Comment: 8 pages, 6 figures, accepted in Ap
Quark Matter 2006: high-pT and jets
An overview of new experimental results on high-\pT{} particle production and
jets in heavy ion collisions from the Quark Matter 2006 conference is
presented.Comment: Presented at Quark Matter 200
Interpreting Magnetic Variance Anisotropy Measurements in the Solar Wind
The magnetic variance anisotropy () of the solar wind has been
used widely as a method to identify the nature of solar wind turbulent
fluctuations; however, a thorough discussion of the meaning and interpretation
of the has not appeared in the literature. This paper explores
the implications and limitations of using the as a method for
constraining the solar wind fluctuation mode composition and presents a more
informative method for interpreting spacecraft data. The paper also compares
predictions of the from linear theory to nonlinear turbulence
simulations and solar wind measurements. In both cases, linear theory compares
well and suggests the solar wind for the interval studied is dominantly
Alfv\'{e}nic in the inertial and dissipation ranges to scales .Comment: 15 pages, 10 figures, accepted for publication in The Astrophysical
Journa
Recommended from our members
Evaluation of materials and surface treatments for the DWPF melter pour spout bellows protective liner
A study was undertaken to evaluate a variety of materials and coatings for the DWPF pour spout bellows liner. The intent was to identify materials that would minimize or eliminate adherence of glass on the bellows liner wall and help minimize possible pluggage during glass pouring operations in DWPF. Glass has been observed adhering to the current bellow`s liner, which is made of 304L stainless steel. Materials were identified which successfully allowed molten glass to hit these surfaces and not adhere. Results of this study suggest that if these materials are used in the pouring system glass could still fall into the canister without appreciable plugging, even if an unstable glass stream is produced. The materials should next be evaluated under the most realistic DWPF conditions possible. Other findings of this study include the following: (1) increasing coupon thickness produced a favorable increase in the glass sticking temperature; (2) highly polished surfaces, with the exception of the oxygen-free copper coupon coated with Armoloy dense chromium, did not produce a significant improvement in the glass sticking temperature, increasing angle of contact of the coupon to the falling glass did not yield a significant performance improvement; (3) electroplating with gold and silver and various diffusion coatings did not produce a significant increase in the glass sticking temperature. However, they may provide added oxidation and corrosion resistance for copper and bronze liners. Boron nitride coatings delaminated immediately after contact with the molten glass
Multiple plasmon resonances in naturally-occurring multiwall nanotubes: infrared spectra of chrysotile asbestos
Chrysotile asbestos is formed by densely packed bundles of multiwall hollow
nanotubes. Each wall in the nanotubes is a cylindrically wrapped layer of . We show by experiment and theory that the infrared spectrum
of chrysotile presents multiple plasmon resonances in the Si-O stretching
bands. These collective charge excitations are universal features of the
nanotubes that are obtained by cylindrically wrapping an anisotropic material.
The multiple plasmons can be observed if the width of the resonances is
sufficiently small as in chrysotile.Comment: 4 pages, 5 figures. Revtex4 compuscript. Misprint in Eq.(6) correcte
- …