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81.
82.
Estimating groundwater storage changes in the Mississippi River basin (USA) using GRACE 总被引:7,自引:0,他引:7
Matthew Rodell Jianli Chen Hiroko Kato James S. Famiglietti Joe Nigro Clark R. Wilson 《Hydrogeology Journal》2007,15(1):159-166
Based on satellite observations of Earth’s time variable gravity field from the Gravity Recovery and Climate Experiment (GRACE), it is possible to derive variations in terrestrial water storage, which includes groundwater, soil moisture, and snow. Given auxiliary information on the latter two, one can estimate groundwater storage variations. GRACE may be the only hope for groundwater depletion assessments in data-poor regions of the world. In this study, soil moisture and snow were simulated by the Global Land Data Assimilation System (GLDAS) and used to isolate groundwater storage anomalies from GRACE water storage data for the Mississippi River basin and its four major sub-basins. Results were evaluated using water level records from 58 wells set in the unconfined aquifers of the basin. Uncertainty in the technique was also assessed. The GRACE-GLDAS estimates compared favorably with the well based time series for the Mississippi River basin and the two sub-basins that are larger than 900,000 km2. The technique performed poorly for the two sub-basins that have areas of approximately 500,000 km2. Continuing enhancement of the GRACE processing methods is likely to improve the skill of the technique in the future, while also increasing the temporal resolution. 相似文献
83.
Takamitsu Yamanaka Yutaka Komatsu Hironori Nomori 《Physics and Chemistry of Minerals》2007,34(5):307-318
Many of ilmenites ABO3 compounds bearing transition elements have semiconductive, ferroelectric and antiferromagnetic properties. The high-pressure
diffraction studies of FeTiO3 have been conducted up to 8.2 GPa using synchrotron radiation in KEK at Tsukuba with diamond anvil cell. The compression
mechanism of FeTiO3 ilmenite has been investigated by the structure refinements converged to the reliable factors R = 0.05. The deformations of the FeO6 and TiO6 octahedra were reduced with increasing pressure. In order to elucidate the electric conductivity change with pressure, electron
density distribution of ilmenite have been executed by maximum entropy method (MEM) using single-crystal diffraction intensity
data. MEM based on F
obs(hkl) of FeTiO3 clearly shows electron density in comparison with the difference Fourier synthesis based on F
obs(hkl) − F
calc(hkl). The radial distribution of the electron density indicates electron localization around the cation positions. The bonding
electron density found in bond Fe–O and Ti–O is lowered with pressure. The isotropic temperature factors B
iso become smaller with increasing pressure. Nevertheless the thermal vibration is considerably restrained by the compression,
the electric conductivity is enhanced with pressure. Neither charge transfer nor electron hopping between Fe and Ti along
the c axis in FeTiO3 is plausible under high pressure. But the electric conductivity due to electron super-exchange in Fe–Fe and Ti–Ti has been
clarified by the MEM electron density distribution. The anisotropy in the electric conductivity has been clarified. 相似文献
84.
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86.
As the origin of the soft X-ray background, emission of soft X-rays from shocks occurred in the accretion of intergalactic gas onto the Galaxy is studied. Infall of discrete gas clouds cannot explain the diffuse component of soft X-rays. If intergalactic gas rich in heavy elements as the cosmic abundance continously flows into the Galaxy and forms a standing shock surrounding the Galaxy, the line emissions by heavy elements from the shocked gas explain the soft X-ray background. Formation of the high velocity cloud by thermal instability in the shocked gas is also discussed briefly. 相似文献
87.
88.
A. Schumann A. Muwanga T. Lehto M. Staudt T. Schlüter V. Kato A. Namboyera 《Geology Today》2015,31(2):59-67
Geosites are important and/or unique geological or geographical features of significance. Typically they comprise geological, palaeontological, as well as archaeological sites. Geosites should be regarded as deserving to be preserved and protected, either from the elements or from destructive human activities, both for the community and future generations. A good knowledge of geological heritage, and a healthy respect for it, is an important factor in the holistic approach for sustainable development. Very often, these sites bear a multi‐faceted ‘story’, which may date back from very recent times to billions of years ago. As such, geosites are of great educational and scientific value. In Africa, such sites have not been receiving the attention they deserve. Only a few countries on the continent acknowledge their importance. Within the framework of a Sustainable Management of Mineral Resources Project (SMMRP), geological mapping, geochemical surveys and mineral resources assessment in selected areas of Uganda have been completed under the umbrella of the Geological Survey of Finland (GTK), and the Department of Geological Survey and Mines (DGSM, Uganda). Apart from recording ‘hard‐tough’ geology, 62 geosites were documented in 2010 and 2011. For the first time, such sites have been incorporated in the new geological maps of the country (at a scale of 1: 250 000). It is possible that this is the first time that such places have been shown on geological maps of Africa. Currently, the extreme north‐east of the country is being geologically mapped by DGSM, with the eventuality of more possible geosites being discovered. 相似文献
89.
We estimate interseismic coupling on the subducting plate interface in the Tokai area, central Japan, by inverting two geodetic data sets. The data record surface motion between March 1996 to May 2000; one represents vertical motion deduced from the leveling observations and the other is the horizontal velocity field deduced from GPS observations. In the inversion, we employed the analytical solutions of surface displacement due to a triangular dislocation element embedded in a homogeneous elastic half space in order to represent the curved plate interface. The vertical data show that the most strongly coupled portion of the subduction interface is concentrated beneath Omaezaki Cape, while the horizontal data show strongest coupling in the shallower region of the subducting plate interface. The estimated maximum value of coupling from the horizontal data is 40 mm/year, while that from vertical data is 25 mm/year. 相似文献
90.
S. Hayakawa T. Kato F. Makino H. Ogawa Y. Tanaka K. Yamashita M. Matsuoka S. Miyamoto M. Oda Y. Ogawara 《Astrophysics and Space Science》1971,12(1):104-117
Cosmic soft X-rays in the energy range between 0.14 and 7 keV were observed with thin polypropylene window proportional counters on board a sounding rocket. The field of view crossed the galactic plane in the Cygnus-Cassiopeia region at a large angle and reached the galactic latitudes of –55° and +30°. Referring also to the result with Be window counters, we obtained the energy spectrum of Cyg XR-2, the flux from the Cas A region and the distribution of the intensity of diffuse X-rays over the scanned region. The turn-over of the Cyg XR-2 spectrum at about 1 keV indicates that the distance of the Cyg XR-2 source lies between 600 and 800 pc, if the turn-over is due entirely to interstellar absorption. The flux from the Cas A region is obtained as 0.23±0.05 photons cm–2 sec–1 in the energy range between 1.1 and 4.1 keV. The intensity of diffuse soft X-rays depends on the galactic latitude more weakly than expected from the interstellar absorption of extragalactic X-rays and shows asymmetry with respect to the galactic equator, thus suggesting a contribution of galactic X-rays. The spectrum of extragalactic X-rays is approximately represented by a power lawE
–1.8. 相似文献