The electronic field shift factor of the 4s2S1/2?4p2PJ transitions in CaII

1993 ◽  
Vol 78 (1-4) ◽  
pp. 247-250 ◽  
Author(s):  
R. E. Silverans ◽  
L. Vermeeren ◽  
A. Klein ◽  
R. Neugart ◽  
C. Schulz ◽  
...  

2019 ◽  
Vol 151 (9) ◽  
pp. 094303 ◽  
Author(s):  
Jack C. Harms ◽  
Leah C. O’Brien ◽  
James J. O’Brien


2018 ◽  
Vol 32 (01) ◽  
pp. 1750359
Author(s):  
Geng-Hua Yu ◽  
Hui Yan ◽  
Jia-Qi Zhong ◽  
Hong Liu ◽  
Xiao-Ling Zhu ◽  
...  

The experimental measurements of the isotope shifts (ISs) for the 1S0–3P1 spin-forbidden transition at 791 nm in neutral barium have been carried out with a thermal barium atom beam. The hyperfine structure (HFS) constants a and b of the odd isotopes [Formula: see text]Ba and [Formula: see text]Ba for this transition have been extracted from the experimental results: a([Formula: see text]Ba) = 1149.9(1.0) MHz, b([Formula: see text]Ba)= −41.6(0.5) MHz, a([Formula: see text]Ba) = 1028.0(1.0) MHz, b([Formula: see text]Ba) = −27.5(0.5) MHz. The measured IS results with the reference isotope [Formula: see text]Ba are 183.7(1.0) MHz ([Formula: see text]Ba–[Formula: see text]Ba), 108.5(0.3) MHz ([Formula: see text]Ba–[Formula: see text]Ba) and 218.9(1.0) MHz ([Formula: see text]Ba–[Formula: see text]Ba). Our IS measurements are in good agreement with the previous experiments. The field shift (FS) factor [Formula: see text] and the mass shift (MS) coefficient [Formula: see text] for this spin-forbidden transition have be determined experimentally as −3.19(4) GHz ⋅ fm[Formula: see text] and −242(20) GHz ⋅ amu, respectively. The results provided herein could be used for further checks theoretically and experimentally, and could also contribute to the study on the nuclear structure of the barium isotopic nuclei.



2021 ◽  
Vol 33 (4) ◽  
pp. 1213-1217 ◽  
Author(s):  
Ekaterina I. Marchenko ◽  
Vadim V. Korolev ◽  
Artem Mitrofanov ◽  
Sergey A. Fateev ◽  
Eugene A. Goodilin ◽  
...  


Geophysics ◽  
2007 ◽  
Vol 72 (1) ◽  
pp. F25-F34 ◽  
Author(s):  
Benoit Tournerie ◽  
Michel Chouteau ◽  
Denis Marcotte

We present and test a new method to correct for the static shift affecting magnetotelluric (MT) apparent resistivity sounding curves. We use geostatistical analysis of apparent resistivity and phase data for selected periods. For each period, we first estimate and model the experimental variograms and cross variogram between phase and apparent resistivity. We then use the geostatistical model to estimate, by cokriging, the corrected apparent resistivities using the measured phases and apparent resistivities. The static shift factor is obtained as the difference between the logarithm of the corrected and measured apparent resistivities. We retain as final static shift estimates the ones for the period displaying the best correlation with the estimates at all periods. We present a 3D synthetic case study showing that the static shift is retrieved quite precisely when the static shift factors are uniformly distributed around zero. If the static shift distribution has a nonzero mean, we obtained best results when an apparent resistivity data subset can be identified a priori as unaffected by static shift and cokriging is done using only this subset. The method has been successfully tested on the synthetic COPROD-2S2 2D MT data set and on a 3D-survey data set from Las Cañadas Caldera (Tenerife, Canary Islands) severely affected by static shift.



1997 ◽  
Vol 22 (1) ◽  
pp. 10-12
Author(s):  
Elizabeth Schmidt
Keyword(s):  




2012 ◽  
Vol 31 (2) ◽  
pp. 8-14
Author(s):  
M. Roa-Villescas ◽  
M. Orozco-Alzate
Keyword(s):  


2016 ◽  
Author(s):  
Xun Wang ◽  
Che-Jen Lin ◽  
Wei Yuan ◽  
Jonas Sommar ◽  
Wei Zhu ◽  
...  

Abstract. Mercury (Hg) emission from natural surfaces plays an important role in global Hg cycling. The present estimate of global natural emission has large uncertainty and remains unverified against field data, particularly for terrestrial surfaces. In this study, a mechanistic model is developed for estimating the emission of elemental mercury vapor (Hg0) from natural surfaces in China. The development implements recent advancements in the understanding of air-soil and air-foliage exchange of Hg0 and redox chemistry in soil and on surfaces, incorporates the effects of soil characteristics and landuse changes by agricultural activities, and is examined through a systematic set of sensitivity simulations. Using meteorology simulated by the Weather Research and Forecasting Model (WRF version 3.7), the exchange of Hg0 between the atmosphere and natural surfaces in Mainland China is estimated to be 465.1 Mg yr−1, including 565.5 Mg yr−1 of emission from soils, 9.0 Mg yr−1 of emission from water body, and 100.4 Mg yr−1 uptake by vegetation. The air-surface exchange is strongly dependent on the landuse and meteorology, with 9 % of net emission from forest ecosystems, 50 % from shrubland, and savanna and grassland, 33 % from cropland, and 8 % from other landuses. Given the large agricultural land area in China, farming activities play an important role on the air-surface exchange in farmland. Particularly, rice field shift from a net sink (3.3 Mg uptake) during April to October (rice planting) to a net source when the farmland is not flooded (November-March). Summing up emissions from each landuse, more than half of the total emission occurs in summer (51 %), followed by spring (28 %), autumn (13 %) and winter (8 %). Model verification is accomplished using observational data of air-soil/air-water fluxes and Hg deposition through litterfall for forest ecosystems in China and Monte Carlo simulations. In contrast to the earlier estimate by Shetty et al. (2008) that reported large emission from vegetative surfaces using an evapotranspiration approach, the estimate in this study shows natural emissions are primarily from grassland and dry cropland. Such an emission pattern may alter the current understanding of Hg emission outflow from China as reported by Lin et al. (2010b) because of a substantial natural Hg emission occurs in West China.



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