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71.
Réka?LukácsEmail author Szabolcs?Harangi Olivier?Bachmann Marcel?Guillong Martin?Dani?ík Yannick?Buret Albrecht?von?Quadt István?Dunkl László?Fodor Jakub?Sliwinski Ildikó?Soós János?Szepesi 《Contributions to Mineralogy and Petrology》2015,170(5-6):52
A silicic ignimbrite flare-up episode occurred in the Pannonian Basin during the Miocene, coeval with the syn-extensional period in the region. It produced important correlation horizons in the regional stratigraphy; however, they lacked precise and accurate geochronology. Here, we used U–Pb (LA-ICP-MS and ID-TIMS) and (U–Th)/He dating of zircons to determine the eruption ages of the youngest stage of this volcanic activity and constrain the longevity of the magma storage in crustal reservoirs. Reliability of the U–Pb data is supported by (U–Th)/He zircon dating and magnetostratigraphic constraints. We distinguish four eruptive phases from 15.9 ± 0.3 to 14.1 ± 0.3 Ma, each of which possibly includes multiple eruptive events. Among these, at least two large volume eruptions (>10 km3) occurred at 14.8 ± 0.3 Ma (Demjén ignimbrite) and 14.1 ± 0.3 Ma (Harsány ignimbrite). The in situ U–Pb zircon dating shows wide age ranges (up to 700 kyr) in most of the crystal-poor pyroclastic units, containing few to no xenocrysts, which implies efficient recycling of antecrysts. We propose that long-lived silicic magma reservoirs, mostly kept as high-crystallinity mushes, have existed in the Pannonian Basin during the 16–14 Ma period. Small but significant differences in zircon, bulk rock and glass shard composition among units suggest the presence of spatially separated reservoirs, sometimes existing contemporaneously. Our results also better constrain the time frame of the main tectonic events that occurred in the Northern Pannonian Basin: We refined the upper temporal boundary (15 Ma) of the youngest counterclockwise block rotation and the beginning of a new deformation phase, which structurally characterized the onset of the youngest volcanic and sedimentary phase. 相似文献
72.
Uta Fritze – von Alvensleben 《Astrophysics and Space Science》2002,281(1-2):379-382
Mergers of massive gas-rich galaxies trigger violent starbursts that - over timescales of > 100 Myr and regions > 10 kpc -
form massive and compact star clusters comparable in mass and radii to Galactic globular clusters. The star formation efficiency
is higher by 1–2 orders of magnitude in these bursts than in undisturbed spirals, irregulars or even BCDs. We ask the question
if star formation in these extreme regimes is just a scaled-up version of the normal star formation mode of if the formation
of globular clusters reveals fundamentally different conditions.
This revised version was published online in September 2006 with corrections to the Cover Date. 相似文献
73.
ISLA will be an astronomical observatory, operating at the upper limit of our planet Earth atmosphere, offering space like
observing conditions in most aspects. ISLA can be maintained easily, modified easily if necessary, always kept at the state
of the art and operated for very extended periods without polluting the stratosphere. ISLA is ideally suited to become the
first world space observatory as the observing conditions are very much space-like – diffraction limited angular resolution,
very low ambient temperature, remote control – however ISLA is easily accessible, telescopes and instruments can be continuously
improved and ISLA's costs corresponds only to those of ground-based modern astronomical installations like the ESO-VLT-, KECK-
and GEMINI-observatories. The cost of observing and experimenting on ISLA will be orders of magnitudes lower than those of
building and operating any space telescope, allowing the astronomers of developing nations to participate in the ISLA observatory
within their limited financial possibilities as competent and full partners. ISLA's 4-m and 2-m telescopes will operate diffraction
limited from 0.3 μm in the optical, over the infrared, far-infrared to the sub-mm spectral range. ISLA's individual telescopes
will permit imaging with 20 milli-arcsec spatial resolution in the optical, 5 times better than the Hubble Space Telescope.
ISLA's telescopes can be combined to form an interferometer with a maximum baseline of 250 m with nearly complete coverage
of the u,v plane. Interferometric resolution will be of the order of 20 micro-arcsec for the optical. ISLA will thus offer
spatial resolution comparable or better than the intercontinental VLBI radio interferometers. ISLA's telescope efficiency
will be many orders of magnitude better than comparable ground-based telescopes. The light collecting power of ISLA's interferometric
telescopes will be orders of magnitudes greater than the future space interferometers under discussion. ISLA, being an aviation
project and not a space project, can be realised in the typical time scale for the development of aviation: about 5 years.
ISLA's cost for the whole observatory, including its movable ground station etc. will be of the order of a typical medium
size ESA space mission. ISLA's lifetime will be in excess of many decades, as it can easily be maintained, modernised, repaired
and improved. ISLA will become the origin of a new astronomical international organisation with worldwide participation. ISLA's
telescopes will be of the greatest importance to all astronomical fields, as it will permit to study much fainter, much more
distant objects with microscopic spatial resolution in wavelength regions inaccessible from ground. ISLA's many telescopes
permit easily simultaneous observations at many wavelengths for rapidly varying objects, from continuously monitoring the
surfaces of the planets in our solar system, surfaces of close-by stars, nuclei of galaxies to QSO's.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
74.
The effect of latitudinal differential heating on the atmospheric general circulation is studied using a simple general circulation model driven by different heating rates. It is found that an increase in differential heating leads to a strengthening of the general circulation as characterized by an increase in global available potential energy, kinetic energy and atmospheric angular momentum. The strengthening of the circulation results in three circulation regimes characterized by different eddy activities. One is a zonally symmetric Hadley regime with no eddy activity while the other two are Rossby regimes dominated by eddies with intermediate and low wave numbers, respectively. Relative to other global indices, the global relative atmospheric angular momentum is superior in detecting the transition of circulation regimes. The regime changes in mid- and high-latitudes resemble the response of the atmosphere to large changes in Earths rotation rate. 相似文献
75.
J. F. Barlow G. G. Rooney S. von Hünerbein S. G. Bradley 《Boundary-Layer Meteorology》2008,127(2):173-191
Profiles of wind and turbulence over an urban area evolve with fetch in response to surface characteristics. Sodar measurements,
taken on 22 April 2002 during the Salford Experiment in the UK (Salfex), are here related to upstream terrain. A logarithmic
layer up to z = 65m was observed in all half-hour averaged profiles. Above this height the profile showed a different vertical gradient,
suggesting a change in surface cover upstream. The drag coefficient varied by a factor of two over only a 20° direction change.
Turbulence intensity (σ
x
) for each wind component (x) decreased with height, but the ratio suggested an underestimate of σ
u
compared to previous results. Mean urban and suburban cover fraction within the source area for each height decreased sharply
between z = 20 and 50m, increasing slightly above. The near-convergence of cover fractions thus occured for source areas of minimum
length ≈ 2,200 m. In comparison, the mean length scale of heterogeneity L
P was calculated from surface cover data to be 1,284 m, and the corresponding mean blending height h
b was 175 m. Finally, the mean streamline angle, α, was negative and the magnitude decreased with height. An exponential fit
to α for z ≤ 65m gave an e-folding height scale of 159 m. A simple relationship between this height scale and L
P was assumed, giving L
P ≈ 1,080 m, which is in reasonable agreement with the estimate from surface cover type. The results suggest that more emphasis
is required on modelling and measuring surface-layer flow over heterogeneous urban canopies. 相似文献
76.
Consistency of observed winter precipitation trends in northern Europe with regional climate change projections 总被引:1,自引:0,他引:1
Often it is claimed that the recent changes in northern European climate are at least partly anthropogenic even though a human
influence has not yet been successfully detected. Hence we investigate whether the recent changes are consistent with regional
climate change projections. Therefore, trends in winter (DJF) mean precipitation in northern Europe are compared to human
induced changes as predicted by a set of four regional climate model simulations. The patterns of recent trends and predicted
changes match reasonably well as indicated by pattern correlation and the similarity is very likely not random. However, the
model projections generally underestimate the recent change in winter precipitation. That is, the signal-to-noise ratio of
the anthropogenic precipitation change is either rather low or the presently used simulations are significantly flawed in
their ability to project changes into the future. European trends contain large signals related to the North Atlantic Oscillation
(NAO), of which a major unknown part may be unrelated to the anthropogenic signal. Therefore, we also examine the consistency
of recent and projected changes after subtracting the NAO signal in both the observations and in the projections. It turns
out that even after the removal of the NAO signal, the pattern of trends in the observations is similar to those projected
by the models. At the same time, the magnitude of the trends is considerably reduced and closer to the magnitude of the change
in the projections. 相似文献
77.
C. Matulla X. Zhang X. L. Wang J. Wang E. Zorita S. Wagner H. von Storch 《Climate Dynamics》2008,30(2-3):133-144
This study examines the performance of the analog method for downscaling daily precipitation. The evaluation is performed
for (1) a number of similarity measures for searching analogs, (2) various ways to include the past atmospheric evolution,
and (3) different truncations in EOF space. It is carried out for two regions with complex topographic structures, and with
distinct climatic characteristics, namely, California’s Central Valley (together with the Sierra Nevada) and the European
Alps. NCEP/NCAR reanalysis data are used to represent the large scale state of the atmosphere over the regions. The assessment
is based on simulating daily precipitation for 103 stations for the month of January, for the years 1950–2004 in the California
region, and for 70 stations in the European Alps (January 1948–2004). Generally, simulated precipitation is in better agreement
with observations in the California region than in the European Alps. Similarity measures such as the Euclidean norm, the
sum of absolute differences and the angle between two atmospheric states perform better than measures which introduce additional
weightings to principal components (e.g., the Mahalanobis distance). The best choice seems dependent upon the target variable.
Lengths of wet spells, for instance, are best simulated by using the angular similarity measure. Overall, the Euclidean norm
performs satisfactorily in most cases and hence is a reasonable first choice, whereas the use of Mahalanobis distance is less
advisable. The performance of the analog method improves by including large-scale information for bygone days, particularly,
for the simulation of wet and dry spells. Optimal performance is obtained when about 85–90% of the total predictor variability
is retained. 相似文献
78.
Near-total depletions of ozone have been observed in the Arctic spring since the mid 1980s. The autocatalytic reaction cycles involving reactive halogens are now recognized to be of main importance for ozone depletion events in the polar boundary layer. We present sensitivity studies using the model MISTRA in the box-model mode on the influence of chemical species on these ozone depletion processes. In order to test the sensitivity of the chemistry under polar conditions, we compared base runs undergoing fluxes of either Br2, BrCl, or Cl2 to induce ozone depletions, with similar runs including a modification of the chemical conditions. The role of HCHO, H2O2, DMS, Cl2, C2H6, HONO, NO2, and RONO2 was investigated. Cases with elevated mixing ratios of HCHO, H2O2, DMS, Cl2, and HONO induced a shift in bromine speciation from Br / BrO to HOBr/HBr, while high mixing ratios of C2H6 induced a shift from HOBr/HBr to Br/BrO. The shifts from Br/BrO to HOBr/HBr accelerated the aerosol debromination, but also increased the total amount of deposited bromine at the surface (mainly via increased deposition of HOBr). For all NOy species studied (HONO, NO2, RONO2) the chemistry is characterized by an increased bromine deposition on snow reducing the amount of reactive bromine in the air. Ozone is less depleted under conditions of high mixing ratios of NOx. The production of HNO3 led to the acid displacement of HCl, and the release of chlorine out of salt aerosol (Cl2 or BrCl) increased. 相似文献
79.
Oskar von der Lühe 《Experimental Astronomy》2009,25(1-3):193-207
Solar observations have been done with telescopes since their invention—already Galileo looked at the Sun. Despite the Sun’s unusual brightness, telescopes which specialize in solar observations are fairly recent, dating from the late nineteenth century onwards. Today, many solar telescopes have rather little in common with nighttime telescopes. They are adapted to high light flux, a limited range of declination, and to the specifications of solar spectrographs and polarimeters. This paper presents the history of the modern optical solar telescope on the ground and in space, the accompanying evolution of scientific capabilities, and a brief outlook into the future. 相似文献
80.
Erosion-driven uplift of the modern Central Alps 总被引:2,自引:0,他引:2
Jean-Daniel Champagnac Fritz Schlunegger Kevin Norton Friedhelm von Blanckenburg Luca M. Abbühl Marco Schwab 《Tectonophysics》2009,474(1-2):236
We present a compilation of data of modern tectono-geomorphic processes in the Central European Alps which suggest that observed rock uplift is a response to climate-driven denudation. This interpretation is predominantly based on the recent quantification of basin-averaged Late Holocene denudation rates that are so similar to the pattern and rates of rock uplift rates as determined by geodetic leveling. Furthermore, a GPS data-based synthesis of Adriatic microplate kinematics suggests that the Central Alps are currently not in a state of active convergence. Finally, we illustrate that the Central Alps have acted as a closed system for Holocene redistribution of sediment in which the peri-Alpine lakes have operated as a sink for the erosional products of the inner Central Alps.While various hypotheses have been put forward to explain Central Alpine rock uplift (e.g. lithospheric forcing by convergence, mantle processes, or ice melting) we show with an elastic model of lithospheric deformation, that the correlation between erosion and rock uplift rates reflects a positive feedback between denudation and the associated isostatic response to unloading. Thus, erosion does not passively respond to advection of crustal material as might be the case in actively converging orogens. Rather, we suggest that the geomorphic response of the Alpine topography to glacial and fluvial erosion and the resulting disequilibrium for modern channelized and associated hillslope processes explains much of the pattern of modern denudation and hence rock uplift. Therefore, in a non-convergent orogen such as the Central European Alps, the observed vertical rock uplift is primarily a consequence of passive unloading due to erosion. 相似文献