1,565 research outputs found
The cultural landscape of megalithic tombs in Denmark, reconstructed by soil pollen analysis
Forty-four pollen spectra from 25 megalithic tombs (5 dolmens and 20 passage graves) in eastern and northern Denmark reveal a highly varied landscape with remains of woodland, coppice woods or secondary woodland and open areas of grass and herb vegetation. Very often there are traces of tree burning. The dominant land-use was cereal growing on burnt sites and pasture. A long-fallow swidden rotation based on the burning of coppice, cereal growing, pasture and coppice regeneration is indicated
New Investigations of Interglacial Fresh-Water Deposits in Jutland: A Preliminary Report
Die Neu-Untersuchung vom „Brörup-Hotel-Moor" und anderer interglazialer Fundstätten aus Jütland haben gezeigt, daß der eigentlichen letzten Interglazialzeit eine kalte Solifluktionsperiode folgte. Ein langes, temperiertes Interstadial mit Birken- und zuletzt auch Fichten- und Föhrenwäldern ging der Hauptphase der letzten Vereisung voraus. Das Interstadial wird dem Göttweiger Interstadial und die vorhergehende kalte Periode dem Altwürm gleichgesetzt. Während der Solifluktionsperiode fanden Umlagerungen von interglazialem Material statt.researc
Infrared properties of SiC particles
We present basic laboratory infrared data on a large number of SiC
particulate samples, which should be of great value for the interpretation of
the 11.3 micron feature observed in the spectra of carbon-rich stars. The
laboratory spectra show a wide variety of the SiC phonon features in the 10-13
micron wavelength range, both in peak wavelength and band shape. The main
parameters determining the band profile are morphological factors as grain size
and shape and, in many cases, impurities in the material. We discovered the
interesting fact that free charge carriers, generated e.g. by nitrogen doping,
are a very common characteristics of many SiC particle samples. These free
charge carriers produce very strong plasmon absorption in the near and middle
infrared, which may also heavily influence the 10-13 micron feature profile via
plasmon-phonon coupling.
We also found that there is no systematic dependence of the band profile on
the crystal type (alpha- vs. beta-SiC). This is proven both experimentally and
by theoretical calculations based on a study of the SiC phonon frequencies.
Further, we give optical constants of amorphous SiC. We discuss the
implications of the new laboratory results for the interpretation of the
spectra of carbon stars.Comment: 17 pages, 12 figures. To appear in A&
Pressure-induced metal-insulator transition in LaMnO3 is not of Mott-Hubbard type
Calculations employing the local density approximation combined with static
and dynamical mean-field theories (LDA+U and LDA+DMFT) indicate that the
metal-insulator transition observed at 32 GPa in paramagnetic LaMnO3 at room
temperature is not a Mott-Hubbard transition, but is caused by orbital
splitting of the majority-spin eg bands. For LaMnO3 to be insulating at
pressures below 32 GPa, both on-site Coulomb repulsion and Jahn-Teller
distortion are needed.Comment: 4 pages, 3 figure
Infrared Spectra of Meteoritic SiC Grains
We present here the first infrared spectra of meteoritic SiC grains. The
mid-infrared transmission spectra of meteoritic SiC grains isolated from the
Murchison meteorite were measured in the wavelength range 2.5--16.5 micron, in
order to make available the optical properties of presolar SiC grains. These
grains are most likely stellar condensates with an origin predominately in
carbon stars. Measurements were performed on two different extractions of
presolar SiC from the Murchison meteorite. The two samples show very different
spectral appearance due to different grain size distributions. The spectral
feature of the smaller meteoritic SiC grains is a relatively broad absorption
band found between the longitudinal and transverse lattice vibration modes
around 11.3 micron, supporting the current interpretation about the presence of
SiC grains in carbon stars. In contrast to this, the spectral feature of the
large (> 5 micron) grains has an extinction minimum around 10 micron. The
obtained spectra are compared with commercially available SiC grains and the
differences are discussed. This comparison shows that the crystal structure
(e.g., beta-SiC versus alpha-SiC) of SiC grains plays a minor role on the
optical signature of SiC grains compared to e.g. grain size.Comment: 7 pages, 6 figures. To appear in A&
Litteratur. Avl og Avlsmetoder.
Litteratur. Avl og Avlsmetoder
Forslag til Præstationsprøver (Trækprøver) for danske Landbrugsheste.
Forslag til Præstationsprøver (Trækprøver) for danske Landbrugsheste
Arbejdsprøve for heste i Finland.
Arbejdsprøve for heste i Finland
Grain size limits derived from 3.6 {\mu}m and 4.5 {\mu}m coreshine
Recently discovered scattered light from molecular cloud cores in the
wavelength range 3-5 {\mu}m (called "coreshine") seems to indicate the presence
of grains with sizes above 0.5 {\mu}m. We aim to analyze 3.6 and 4.5 {\mu}m
coreshine from molecular cloud cores to probe the largest grains in the size
distribution. We analyzed dedicated deep Cycle 9 Spitzer IRAC observations in
the 3.6 and 4.5 {\mu}m bands for a sample of 10 low-mass cores. We used a new
modeling approach based on a combination of ratios of the two background- and
foreground-subtracted surface brightnesses and observed limits of the optical
depth. The dust grains were modeled as ice-coated silicate and carbonaceous
spheres. We discuss the impact of local radiation fields with a spectral slope
differing from what is seen in the DIRBE allsky maps. For the cores L260,
ecc806, L1262, L1517A, L1512, and L1544, the model reproduces the data with
maximum grain sizes around 0.9, 0.5, 0.65, 1.5, 0.6, and > 1.5 {\mu}m,
respectively. The maximum coreshine intensities of L1506C, L1439, and L1498 in
the individual bands require smaller maximum grain sizes than derived from the
observed distribution of band ratios. Additional isotropic local radiation
fields with a spectral shape differing from the DIRBE map shape do not remove
this discrepancy. In the case of Rho Oph 9, we were unable to reliably
disentangle the coreshine emission from background variations and the strong
local PAH emission. Considering surface brightness ratios in the 3.6 and 4.5
{\mu}m bands across a molecular cloud core is an effective method of
disentangling the complex interplay of structure and opacities when used in
combination with observed limits of the optical depth.Comment: 23 pages, 18 figures, accepted for publication in A&
Momentum-resolved spectral functions of SrVO calculated by LDA+DMFT
LDA+DMFT, the merger of density functional theory in the local density
approximation and dynamical mean-field theory, has been mostly employed to
calculate k-integrated spectra accessible by photoemission spectroscopy. In
this paper, we calculate k-resolved spectral functions by LDA+DMFT. To this
end, we employ the Nth order muffin-tin (NMTO) downfolding to set up an
effective low-energy Hamiltonian with three t_2g orbitals. This downfolded
Hamiltonian is solved by DMFT yielding k-dependent spectra. Our results show
renormalized quasiparticle bands over a broad energy range from -0.7 eV to +0.9
eV with small ``kinks'', discernible in the dispersion below the Fermi energy.Comment: 21 pages, 8 figure
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