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1.
We present a software package developed for the automatic 4-D stellar parameterization. The package can be adopted to virtually
any multicolour photometric system. Procedure of simultaneous determination of T
eff, log g, [M/H] and E
B-V is very flexible and can be performed by applying various photometric parameters(magnitudes, colour indices etc.). Any changes
of the photometric systems, weighting schemes or parameterization criteria can be implemented easily.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
2.
Enhanced Taurid activity in terms of visual meteor and fireball rates has been found in 1988, 1991, 1995, 1998 and 2005 data. The years of heightened activity are shown to be unequivocally linked to the encounters of swarms of resonantly trapped particles in the Taurid meteoroid stream according to the model proposed by Asher & Clube. While the annual activity level of the Taurid meteor shower in terms of zenithal hourly rate (ZHR) is 7.8 ± 1.2 , swarm year activity typically reaches ZHRs of 12–17. The annual fraction of fireballs is below 1 per cent; in swarm years, this fraction is as high as 2.4–4.6 per cent near the maximum of the Taurid activity period. 相似文献
3.
Anisotropy of magnetic susceptibility and structural geology of the ca. 1.45 Ga Karlshamn pluton (southern Sweden) are used
to study its emplacement and structural evolution. The Karlshamn pluton is one of the largest metaluminous A-type granitoid
intrusions in southern Sweden. It is a multiphase body made up of two suites that differ in composition but which have similar
crystallization ages. The magmatic foliation, ductile shear zones and granite–pegmatite filled fractures were mapped as well
as the metamorphic foliation and extension lineation in the metamorphic host rocks. The anisotropy of magnetic susceptibility
was used to map the magnetite petrofabric of the pluton, providing a larger data set for both the magmatic foliations and
lineations, which could not be mapped in the field. The fabrics within the pluton are continuous with the metamorphic fabrics
in the country rocks. Both the pluton and the country rock fabrics were folded during ENE–WSW compression, while the pluton
was still a magma mush. The stress field orientation during cooling of the pluton is determined on the basis of magmatic,
ductile and brittle structures in the Karlshamn pluton that formed successively as the pluton cooled. The compressional event
is referred to as the Danopolonian orogeny and therefore the Karlshamn granitoids, and other plutons of similar composition
and age in central and southern Sweden, on the Danish Island of Bornholm, and in Lithuania, may be considered as syntectonic
intrusions and not as anorogenic, as was previously thought. 相似文献
4.
Jokūbas Sūdžius Saulius Raudeliūnas Arūnas Kučinskas Audrius Bridžius Vladas Vansevičius 《Astrophysics and Space Science》2002,280(1-2):109-114
We investigate the possibilities for tracing interstellar extinction with the ESA's astrometric space mission GAIA. The analysis
is based on detailed simulations of the GAIA photometry, which are used to derive the distribution of interstellar matter
in a modelled Galaxy. We find that `small' diffuse clouds (diameter D = 4 pc, E
B-V = 0.06) will be easily traced with GAIA up to the distances of ∼ 800 pc. `Large' diffuse interstellar clouds (D = 10 pc, E
B-V = 0.13) will be located up to the distances of ∼ 2.5 kpc. This holds for the reddening tracers of spectral types O – K2 brighter
than V = 17. Inmost cases, due to their low spatial density, the early type stars (O– A2) cannot provide reliable information about
the distribution of interstellar matter. None of the reddening tracers measured by GAIA will provide reliable identification
of the individual interstellar clouds beyond the distances of ∼ 3 kpc. Therefore, we conclude that the information available
from photometric observations will be not sufficient for the detailed reconstruction of the 3-D distribution of Galactic interstellar
matter. It is therefore extremely important to define the new strategies which would allow to combine all the available information,
including the earlier space- and/or ground-based investigations, together with the information which will be provided by GAIA
itself (parallaxes, E
B-V etc.).
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
5.
Algirdas Kazlauskas Vladas Vansevičius Audrius Bridžius Ramutis Drazdys Romualdas Kalytis 《Astrophysics and Space Science》2002,280(1-2):57-62
We investigate the effects arising from the filter transmission curve differences across the filter area in the 3G medium-band
photometric system proposed for GAIA. We discuss the accuracy of the transformations to the standard photometric system and
the precision of the determination of physical parameters for various types of stars using the 4-D classification procedure.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
6.
P. Dalin N. Pertsev S. Frandsen O. Hansen H. Andersen A. Dubietis R. Balciunas 《Journal of Atmospheric and Solar》2010,72(14-15):1129-1138
Bright and extensive noctilucent clouds (NLC) were observed in Århus (Denmark) on 3/4 July of 2008 with an automatic digital camera taking images every minute. This event was unique in the sense that bright NLC were seen at high elevation angles (more than 30°) that allowed observing the evolution of a Kelvin–Helmholtz (KH) wave, resulted in well-developed turbulence. In particular, coherent vortex structures of a horseshoe-shaped form were observed for the first time in noctilucent clouds. The turbulent diffusion coefficient and turbulent energy dissipation rate around the mesopause are estimated in the range 162–667 m2/s and 300–1235 mW/kg, respectively, representing a case of strong neutral air turbulence in noctilucent clouds. Turbulent structures were observed to be in the vicinity of breaking small-scale gravity waves that seems to be responsible for a high level of turbulence.At the same time, it has been demonstrated that it is of importance to take into account non-turbulent process such as the gravity wave motion that is always present in NLC layers. Unless non-turbulent process is taken into account, this certainly leads to overestimating of the value of the turbulent diffusion coefficient. More accurate characteristics of turbulence in NLC can be obtained by analyzing a sequence of high-resolution images with a high frame-rate high-resolution digital camera. 相似文献
7.
Arūnas Kučinskas Audrius Bridžius Vladas Vansevičius 《Astrophysics and Space Science》2002,280(1-2):159-163
The goal of this work is to assess the expected scientific output from the photometric studies of globular clusters in the
Large Magellanic Cloud with ESA's astrometric space mission GAIA. For this purpose we simulate GAIA photometry of individual
stars in synthetic cluster populations, covering a large range of cluster ages and metallicities. We find that accurate effective
temperatures (Δ T
eff<10%) can be obtained from GAIA photometry down to V ∼ 18 for stars in populations within the studied metallicity range ([M/H] = -0.4 ... -1.7). GAIA will also provide photometric
metallicities (Δ [M/H] ≲ 0.3 dex) for the cluster giants brighter than V ∼ 17.5. The knowledge of the effective temperature sand metallicities will allow to obtain accurate ages of stellar populations
younger than about 1 Gyr using the usual procedure of main sequence turn-off point fitting. Ages of older stellar populations
(≳ 1 Gyr) may be constrained from the isochrone fits to the giant branches in the observed CMDs. We conclude that GAIA will
provide excellent opportunities for studying star formation histories far beyond the Milky Way, providing means for better
understanding of stellar and galactic evolution in different astrophysical environments.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
8.
Vladas Vansevičius Audrius Bridžius Ramutis Drazdys 《Astrophysics and Space Science》2002,280(1-2):31-39
We present a method and results of evaluation of the photometric systems (PSs) proposed for the GAIA mission. The method,
however, can be applied for the analysis of virtually any multicolour PS designed for the global investigation of the Galactic
stellar populations. Performance of the 1F, 2A and 3G PSs is evaluated taking into account their ability to simultaneously
determine the main stellar parameters,T
eff, log g, [M/H] and E
B-V, for a large variety of stars down to G ∼ 20. The representative Galactic stellar populations were constructed and employed for evaluation of the PSs. Despite the
fact that the 2A and 3G PSs perform significantly better than the 1F (presently adopted as a baseline PS for GAIA), we conclude
that still there is no photometric system proposed to date, which would allow to achieve the scientific objectives of the
GAIA mission.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
9.
Vladas Vansevi?ius Audrius Brid?ius Ramutis Drazdys 《Astrophysics and Space Science》2002,279(4):419-421
Volume Contents
Volume contents 相似文献10.
Audrius Dubietis Peter Dalin Ričardas Balčiūnas Kazimieras Černis 《Journal of Atmospheric and Solar》2010,72(14-15):1090-1099
We present an analysis of systematic visual and photographic observations of noctilucent clouds seen from Lithuania in the years 1973–2009. The main trends in the noctilucent cloud occurrence frequency and the mean brightness are derived from statistical and correlation analysis. A clear signature of the solar activity cycle is imprinted on the noctilucent cloud occurrence frequency and mean brightness, both showing distinct anti-correlation with the sunspot numbers; however, no statistically significant increase of either noctilucent cloud occurrence frequency or brightness has been detected at least over past 19 yr (1991–2009). The only statistically significant positive trend is established for the numbers of very bright noctilucent cloud displays in the years 1973–2009. The most recent noctilucent cloud observations are linked to variations of local mesospheric temperatures, measured by the Aura satellite. 相似文献