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141.
Optical long-baseline interferometry is a unique and powerful technique for astronomical research. Since the 1980’s (with I2T, GI2T, Mark I to III, SUSI, ...), optical interferometers have produced an increasing number of scientific papers covering various fields of astrophysics. As current interferometric facilities are reaching their maturity, we take the opportunity in this paper to summarize the conclusions of a few key meetings, workshops, and conferences dedicated to interferometry. We present the most persistent recommendations related to science cases and discuss some key technological developments required to address them. In the era of extremely large telescopes, optical long-baseline interferometers will remain crucial to probe the smallest spatial scales and make breakthrough discoveries. 相似文献
142.
Philippe André 《Astrophysics and Space Science》2002,281(1-2):51-66
Detailed studies of nearby cluster-forming molecular clouds can help us understand the physical processes by which most stars
form in galaxies. I review recent advances made on this subject. Submillimeter observations of nearby protoclusters suggest
that stars are generally built from finite, detached reservoirs of mass inside molecular cloud cores, and point to a cloud
fragmentation origin for the IMF. Much progress in this field will come from future large submillimeter instruments such as
Herschel and ALMA.
This revised version was published online in September 2006 with corrections to the Cover Date. 相似文献
143.
In this work 13 Planetary Nebulae have been classified as Type I according to Peimbert's criteria (Peimbert, 1978). These objects have been added to a previous sample (Maciel and Faúndez-Abans, 1985) and diagrams of O/H versus N/H, S/H, Ne/H and Ar/H, as well as N/H versus S/H, Ne/H and Ar/H have been drawn. All of them exhibit a tendency for linear correlation; moreover, the behavior of O and N versus Ar and S are very similar, with approximately the same slope. When the excitation class parameter was included in the diagrams, no clear tendency can be discerned, for any class. 相似文献
144.
E. Lohinger C. Froeschlé R. Dvorak 《Celestial Mechanics and Dynamical Astronomy》1993,56(1-2):315-322
The Lyapunov characteristic numbers (LCNs) which are defined as the mean value of the distribution of the local variations of the tangent vectors to the flow (=ln
k
i
) (see Froeschlé, 1984) have been found to be sensitive indicators of stochasticity. So we computed the distribution of these local variations and determined the moments of higher order for the integrable and stochastic regions in a binary star system with =0.5. 相似文献
145.
A. Deutsch R. A. F. Grieve M. Avermann L. Bischoff P. Brockmeyer D. Buhl R. Lakomy V. Müller-Mohr M. Ostermann D. Stöffler 《International Journal of Earth Sciences》1995,84(4):697-709
The occurrence of shock metamorphic features substantiates an impact origin for the 1.85 Ga old Sudbury Structure, but this has not been universally accepted. Recent improvements in knowledge of large-scale impact processes, combined with new petrographic, geochemical, geophysical (LITHOPROBE) and structural data, allow the Sudbury Structure to be interpreted as a multi-ring impact structure. The structure consists of the following lithologies: Sudbury Breccia —dike breccias occurring up to 80 km from the Sudbury Igneous Complex (SIC); Footwall rocks and Footwall Breccia — brecciated, shocked crater floor materials, in part thermally metamorphosed by the overlying SIC; Sublayer and Offset Dikes, Main Mass of the SIC and Basal Member of the Onaping Formation (OF) — geochemically heterogeneous coherent impact melt complex ranging from inclusion-rich basal unit through a dominantly inclusion-free to a capping inclusion-rich impact melt rock; Grey Member of OF — melt-rich impact breccia (suevite); Green Member of OF — thin layer of fall back ejecta; Black Member of OF — reworked and redeposited breccia material; Onwatin and Chelmsford Formations — post-impact sediments. Observational and analytical data support an integrated step-by-step impact model for the genesis of these units. Analysis of the present spatial distribution of various impact-related lithologies and shock metamorphic effects result in an estimated original rim-to-rim diameter of the final crater of 200 or even 280 km for the Sudbury Structure, prior to tectonic thrusting and deformation during the Penokean orogeny. 相似文献
146.
Influence of shallow infiltration on time-lapse ERT: Experience of advanced interpretation 总被引:1,自引:0,他引:1
Rémi Clément Marc Descloitres Thomas Günther Olivier Ribolzi Anatoli Legchenko 《Comptes Rendus Geoscience》2009,341(10-11):886-898
Previous time-lapse Electrical Resistivity Tomography (ERT) studies have experienced difficulties in reconstructing reliable calculated resistivity changes in the subsurface. Increases or decreases of resistivity appear in the calculated ERT image where no changes were noted in the subsurface, leading to erroneous hydrological interpretations of the geophysical results. In this article, we investigate how a variation of actual resistivity with time and at shallow depth can influence time-lapse ERT results and produce resistivity artefacts at depth. We use 1 and 2-D numerical modelling to simulate infiltration scenarios. Using a standard time-lapse inversion, we demonstrate the resistivity artefact production according to the electrode spacing parameter. We used an advanced inversion methodology with a decoupling line at shallow depth to attenuate or remove resistivity artefacts. We also applied this methodology to a field data set obtained in a semi-arid environment in Burkina Faso, West Africa. Here, time-lapse ERT shows several resistivity artefacts of calculated resistivity if a standard inversion is used. We demonstrate the importance of a dense sampling of shallow resistivity variations at shallow depth. Advanced interpretation allows us to significantly attenuate or remove the resistivity artefact production at intermediate depth and produce reliable interpretation of hydrological processes. 相似文献
147.
Sébastien Couvidat S. P. Rajaguru Richard Wachter K. Sankarasubramanian Jesper Schou Philip H. Scherrer 《Solar physics》2012,278(1):217-240
The Helioseismic and Magnetic Imager (HMI) instrument onboard the Solar Dynamics Observatory produces line-of-sight (LOS) observables (Doppler velocity, magnetic-field strength, Fe i line width, line depth, and continuum intensity) as well as vector magnetic-field maps at the solar surface. The accuracy of LOS observables is dependent on the algorithm used to translate a sequence of HMI filtergrams into the corresponding observables. Using one hour of high-cadence imaging spectropolarimetric observations of a sunspot in the Fe i line at 6173 Å through the Interferometric Bidimensional Spectrometer installed at the Dunn Solar Telescope, and the Milne–Eddington inversion of the corresponding Stokes vectors, we test the accuracy of the observables algorithm currently implemented in the HMI data-analysis pipeline: the MDI-like algorithm. In an attempt to improve the accuracy of HMI observables, we also compare this algorithm to others that may be implemented in the future: a least-squares fit with a Gaussian profile, a least-squares fit with a Voigt profile, and the use of second Fourier coefficients in the MDI-like algorithm. 相似文献
148.
The shielding effect of plasma on the electrostatic potential due to a central nucleus is studied. The potential is determined by the Poisson equation with Boltzmann factor for the charge density of ions. The aim of this work is to find approximated analytical solutions, without the usual linearization hypothesis, by means of the technique of quasifractional approximants in two points. In a previous work (Martín and Pérez, 1994) a quasifractional fractional approximation was obtained, but the coefficients were found by means of the numerical solution of the differential equation. Now we find a complete analytical expression. The approximant found is highly precise in the range of validity of the physical model used. 相似文献
149.
We present a study at HST-like spatial resolution of the gas kinematics in the innermost part of NGC 1068. This work is based
on observations with the integral field spectrograph TIGER mounted on the CFH Telescope. We first derived the final spatial
PSF of our data and checked its photometric integrity by comparison with two independent [OIII] HST images (FOC and WFPC2).
We then performed a spatial deconvolution of the data-cube constraining the sum of the deconvolved velocity-slices to be as
close as possible to the HST image. The resulting deconvolved data-cube has then a resolution similar to the HST image. It
shows that the velocity distribution of the inner clouds detected with the HST differs strongly from a simple NE-SW ejection
flow. We thus show that the previous interpretations of the double-peaked lines NE of the nucleus must be revisited.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
150.
The Portneuf–Mauricie Domain (PMD), located in the south-central part of the Grenville province, contains Mesoproterozoic
Ni–Cu ± platinum-group element (PGE) prospects hosted in a variety of plutonic intrusions (layered, with simple structures,
or zoned) and emplaced in a mature island arc setting. A two-stage model is envisaged to explain the formation of magmatic
sulfides. An early loss of a small amount of sulfides in the conduits of primitive, hydrous mantle-derived melts under high
fO2, resulted in depletion of the magmas in chalcophile and precious metals (Cu/Pd ratios vary from initial mantle values up
to 1.6 × 106). Then, nearer the mineralized zones, the magmas interacted with sulfide-bearing country rocks, resulting in felsification
of the magmas, assimilation of crustal sulfur (δ
34S values up to +5.5‰), and the formation of an immiscible sulfide liquid. Liquid-sulfide formation was followed by variable
interactions between the silicate and sulfide magmas, which were responsible for the enrichment of sulfides in Ni, Cu, and,
locally, PGE. Indeed, low R factors are found for prospects hosted in intrusions with a simple internal structure and in layered intrusions whereas high
R factors are found for prospects hosted in zoned intrusions. Finally, sulfide melt may have been partly incorporated into
later pulses of magma and injected into shallow magma chambers to form the PMD prospects. The PMD prospects share common characteristics
with other well-known deposits (Aguablanca, Vammala, Stormyrplunen, and deposits in Alaskan/Ural-type intrusions), attesting
to the Ni, Cu, and PGE potential of deposits associated with subduction-zone settings. 相似文献