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51.
R. Lambert 《Theoretical and Applied Climatology》1992,45(1):83-88
Summary Research carried out on a favourable site in the Pre-Alps of Savoy has allowed the development of risk cartography where avalanche phenomena are defined according to three criteria: maximum extension, type of avalanche, and frequency of avalanche. The maps, composed of simple symbols, allowing easy updating, could be a useful tool for mountain professionals.With 4 Figures 相似文献
52.
M. H. Slovak J. P. Cassinelli C. M. Anderson D. L. Lambert 《Astrophysics and Space Science》1987,131(1-2):765-769
Satellite observations, fromEinstein,IUE, andIRAS, have been combined with ground-based observations to derive the quiescent energy distribution of the symbiotic star AG Draconis. A detailed comparison is made between the combined observations and various steady-state composite models, including blackbody accretion disks.Paper presented at the IAU Colloquium No. 93 on Cataclysmic Variables. Recent Multi-Frequency Observations and Theoretical Developments, held at Dr. Remeis-Sternwarte Bamberg, F.R.G., 16–19 June, 1986. 相似文献
53.
David L. Lambert Andrew McWilliam Verne V. Smith 《Astrophysics and Space Science》1987,133(2):369-381
High-resolution spectra near 4 m of the four red giants— Peg,o
1 Ori, 10 Dra, and HR 1105—have been analysed to obtain estimates of the28Si/29Si and28Si/30Si abundance ratios. For Peg and the S star HR 1105, the28Si/29Si ratio is close to the solar ratio (28Si/29Si=20).29Si appears to be underabundant in the MS staro
1 Ori (28Si/29Si=40) and the M star 10 Dra (28Si/29Si53). The30Si isotope appears to be underabundant by, perhaps, about a factor of 2 in all four stars. 相似文献
54.
L. S. Lyubimkov S. I. Rostopchin T. M. Rachkovskaya D. B. Poklad D. L. Lambert 《Monthly notices of the Royal Astronomical Society》2005,358(1):193-201
From high-resolution spectra a non-local thermodynamic equilibrium analysis of the Mg ii 4481.2-Å feature is implemented for 52 early and medium local B stars on the main sequence (MS). The influence of the neighbouring line Al iii 4479.9-Å is considered. The magnesium abundance is determined; it is found that log ɛ(Mg) = 7.67 ± 0.21 on average. It is shown that uncertainties in the microturbulent parameter Vt are the main source of errors in log ɛ(Mg) . When using 36 stars with the most reliable Vt values derived from O ii and N ii lines, we obtain the mean abundance log ɛ(Mg) = 7.59 ± 0.15 . The latter value is precisely confirmed for several hot B stars from an analysis of the Mg ii 7877-Å weak line. The derived abundance log ɛ(Mg) = 7.59 ± 0.15 is in excellent agreement with the solar magnesium abundance log ɛ⊙ (Mg) = 7.55 ± 0.02 , as well as with the proto-Sun abundance log ɛ ps (Mg) = 7.62 ± 0.02 . Thus, it is confirmed that the Sun and the B-type MS stars in our neighbourhood have the same metallicity. 相似文献
55.
Hernandez-Mora Marina Meseguer-Ruiz Oliver Karas Cyrus Lambert Fabrice 《Natural Hazards》2021,109(3):2153-2171
Natural Hazards - Human settlements in coastal areas are highly vulnerable to extreme events, especially in the Mediterranean area, which houses a large number of tourists during the summer and... 相似文献
56.
The energy cycle characterizes basic aspects of the physical behaviour of the climate system. Terms in the energy cycle involve
first and second order climate statistics (means, variances, covariances) and the intercomparison of energetic quantities
offers physically motivated “second order” insight into model and system behaviour. The energy cycle components of 12 models
participating in AMIP2 are calculated, intercompared and assessed against results based on NCEP and ERA reanalyses. In general,
models simulate a modestly too vigorous energy cycle and the contributions to and reasons for this are investigated. The results
suggest that excessive generation of zonal available potential energy is an important driver of the overactive energy cycle
through “generation push” while excessive dissipation of eddy kinetic energy in models is implicated through “dissipation
pull‘’. The study shows that “ensemble model” results are best or among the best in the comparison of energy cycle quantities
with reanalysis-based values. Thus ensemble approaches are apparently “best” not only for the simulation of 1st order climate
statistics as in Lambert and Boer (Clim Dyn 17:83–106, 2001) but also for the higher order climate quantities entering the
energy cycle. 相似文献
57.
58.
Lambert Wanninger 《GPS Solutions》2009,13(2):133-139
Antenna changes at GNSS reference stations frequently produce discontinuities in the coordinate time series. These apparent
position shifts are mainly caused by changes of carrier-phase multipath effects and different errors in the antenna phase
center corrections. A monitoring method was developed and successfully tested, which requires additional GNSS observations
from a local, temporary reference station. Changes of carrier-phase measurement errors due to the antenna change are determined
and stored in L1 and L2 phase maps. These phase maps provide corrections to be applied either to the observation data obtained
before the antenna change or to the observation data obtained after the antenna change. The observation corrections are able
to remove coordinate discontinuities independent of the selected coordinate estimation algorithm.
相似文献
Lambert WanningerEmail: |
59.
M.L. Filippi P. Lambert J. Hunziker B. Kübler S. Bernasconi 《Journal of Paleolimnology》1999,21(1):19-34
Lake Neuchåtel is a medium sized, hard-water lake, lacking varved sediments, situated in the western Swiss Lowlands at the foot of the Jura Mountains. Stable isotope data (18O and 13C) from both bulk carbonate and ostracode calcite in an 81 cm long, radiocarbon-dated sediment core represent the last 1500 years of Lake Neuchåtel's environmental history. Comparison between this isotopic and other palaeolimnologic data (mineralogical, geochemical, palynological, etc.) helps to differentiate between anthropogenic and natural factors most recently affecting the lake. An increase in lacustrine productivity (450–650AD ca), inferred from the positive trend in 13C values of bulk carbonate, is related to medieval forest clearances and the associated nutrient budget changes. A negative trend in both the bulk carbonate and ostracode calcite 18O values between approximately 1300 and 1500AD, is tentatively interpreted as due to a cooling in mean air temperature at the transition from the Medieval Warm Period to the Little Ice Age. Negative trends in bulk carbonate 18O and 13C values through the uppermost sediments, which have no equivalent in ostracode calcite isotopic values, are concomitant with the recent onset of eutrophication in the lake. Isotopic disequilibrium during calcite precipitation, probably due to kinetic factors in periods of high productivity is postulated as the mechanism to explain the associated negative isotopic trends, although the effect of a shift of the calcite precipitation towards the warmer months cannot be excluded. 相似文献
60.