1,957,644 research outputs found
Statistical separability and classification of land use classes using image-100
The author has identified the following significant results. The statistical separability of land use classes in the subsets of one to four spectral channels was investigated. Using ground observations and aerial photography, the MSS data of LANDSAT were analyzed with the Image-100. In the subsets of one to three spectral channels, channel 4, channel 4 & 7, and channels 4, 5, & 7 were found to be the best choices (ch.4 - 0.5 to 0.6 microns, ch. 5 - 0.6 to 0.7 microns, ch. 6 - 0.7 to 0.8 microns, and ch. 7 - 0.8 to 1.1 microns). For the single cell option of the Image-100, the errors of omission varied from 5% for the industrial class to 46% for the institutional class. The errors of commission varied from 11% for the commercial class to 39% for the industrial class. On the whole, the sample classifier gave considerably more accurate results compared to the single cell or multicell option
Effect of CH addition on excess electron mobility in liquid Kr
The excess electrons mobility has been measured recently in liquid
mixtures of Kr and CH as a function of the electric field up to and of the CH concentration up to at
temperatures fairly close to the normal boiling point of Kr
(folegani). We present here new data which extend the
previous set in the region of low electric field. The experimental results are
interpreted in terms of a kinetic model previously proposed to explain the
concentration dependent behavior of in liquid Ar--Kr and Ar--Xe mixtures.
The main result is that CH is more effective in enhancing
energy--transfer rather than momentum--transfer in comparison with mixtures of
liquified noble gases. The field dependence of is quite complicate. In
particular, at intermediate values of the field, there appears to be a
crossover between two different electric--field dependent behaviors of
The electric field strength at crossover is well correlated with the
concentration of CH This fact suggests that different excitations of the
molecular solute might be involved in the momentum-- and energy--transfer
processes for different values of the mean electron energy.Comment: 17, pages,7 figures, RevTeX4, submitted to J.Chem.Phy
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Methane (CH<sub>4</sub>) flux data for Moidach More. Years 1997 - 1998
Methane (CH4) emission data collected from an extensive pristine portion of raised peat bog located in Moidach More, Morayshire, northeast Scotland (UK). CH4 flux was measured using static chambers, which were sampled on a weekly (late spring to early autumn) to monthly basis (late autumn to early spring), starting in May 1997
Spectroscopic parameters and rest frequencies of isotopic methylidynium, CH+
Astronomical observations toward Sagittarius B2(M) as well as other sources
with APEX have recently suggested that the rest frequency of the J = 1 - 0
transitions of 13CH+ is too low by about 80 MHz. Improved rest frequencies of
isotopologs of methylidynium should be derived to support analyses of spectral
recording obtained with the ongoing Herschel mission or the upcoming SOFIA.
Laboratory electronic spectra of four isotopologs of CH+ have been subjected to
one global least-squares fit. Laboratory data for the J = 1 - 0 ground state
rotational transitions of CH+, 13CH+, and CD+, which became available during
the refereeing process, have been included in the fit as well. An accurate set
of spectroscopic parameters has been obtained together with equilibrium bond
lengths and accurate rest frequencies for six CH+ isotopologs: CH+, 13CH+,
13CD+, CD+, 14CH+, and CT+. The present data will be useful for the analyses of
or SOFIA observations of methylidynium isotopic species.Comment: Astronomy and Astrophysics, accepted as Letter; 4 (here 5) page
Sensitivity analysis of a wetland methane emission model based on temperate and arctic wetland sites
Modelling of wetland CH<sub>4</sub> fluxes using wetland soil emission models is used to determine the size of this natural source of CH<sub>4</sub> emission on local to global scale. Most process models of CH<sub>4</sub> formation and soil-atmosphere CH<sub>4</sub> transport processes operate on a plot scale. For large scale emission modelling (regional to global scale) upscaling of this type of model requires thorough analysis of the sensitivity of these models to parameter uncertainty. We applied the GLUE (Generalized Likelihood Uncertainty Analysis) methodology to a well-known CH<sub>4</sub> emission model, the Walter-Heimann model, as implemented in the PEATLAND-VU model. The model is tested using data from two temperate wetland sites and one arctic site. The tests include experiments with different objective functions, which quantify the fit of the model results to the data. <br><br> The results indicate that the model 1) in most cases is capable of estimating CH<sub>4</sub> fluxes better than an estimate based on the data avarage, but does not clearly outcompete a regression model based on local data; 2) is capable of reproducing larger scale (seasonal) temporal variability in the data, but not the small-scale (daily) temporal variability; 3) is not strongly sensitive to soil parameters, 4) is sensitive to parameters determining CH<sub>4</sub> transport and oxidation in vegetation, and the temperature sensitivity of the microbial population. The GLUE method also allowed testing of several smaller modifications of the original model. <br><br> We conclude that upscaling of this plot-based wetland CH<sub>4</sub> emission model is feasible, but considerable improvements of wetland CH<sub>4</sub> modelling will result from improvement of wetland vegetation data
Spectropolarimetric observations of cool DQ white dwarfs
Following our recent discovery of a new magnetic DQ white dwarf (WD) with CH
molecular features, we report the results for the rest of the DQ WDs from our
survey. We use high signal-to-noise spectropolarimetric data to search for
magnetic fields in a sample of 11 objects. One object in our sample,
WD1235+422, shows the signs of continuum circular polarization that is similar
to some peculiar DQs with unidentified molecular absorption bands, but the low
S/N and spectral resolution of these data make more observations necessary to
reveal the true nature of this object.Comment: 4 pages, 4 figures. Accepted for publication in Astronomy &
Astrophysic
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