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deep core
Regarding nonreciprocal activity, one should be cautious about discussing magnetic symmetry because the deep core hole can couple the true ground state with low-lying excited states.
      
Theory of intrinsic and extrinsic excitation effects in deep core XPS spectra studied by the many-body scattering theory
      
Intrinsic and extrinsic energy loss structures observed in XPS spectra from a deep core are discussed based on the many-body scattering theory proposed by Fukutome and Low.
      
Lifetime effects on the intrinsic and extrinsic excitation in deep core XPS and X-ray absorption spectra
      
The lifetime effects of the core hole are taken into account in order to investigate the deep core XPS and X-ray absorption spectra in the theoretical framework developed by the present author.
      
We discuss how to analyze these valence band and deep core level excitation spectra, concerning particularly with which orbital, Cud or Op state, a hole will occupy in the CuO2 plane.
      
These data and that from a single deep core demonstrate that the estuary was polluted from mining activity long before the large-scale operations began in the late nineteenth century.
      
A 90?m deep core from the Massaciuccoli lake basin (Tuscany, Italy) offers new material for improving the knowledge of the Holocene vegetation history in the coastal plains in Tuscany and Liguria bordering the Mar Ligure (Ligurian sea).
      
Time control of the 196 m deep core was based on 11 finite 14C dates in the upper 17 m, magnetostratigraphy and correlation with the marine oxygen isotope stratigraphy.
      
We evaluated the cooling rate of hyperthermic subjects, as measured by three estimates of deep core temperatures (esophageal, rectal and aural canal temperatures), during immersion in a range of water temperatures.
      
End of survival is marked by the deep core temperature reaching a value of 30° C.
      
The typical velocity in the Equatorial Undercurrent (EU) deep core is about 20 cm/s.
      
Effects of spinal anesthesia on the peripheral and deep core temperature in elderly diabetic patients undergoing urological surg
      
SOHO, the Solar and Heliospheric Observatory, is a project of international cooperation between ESA and NASA to study the Sun, from its deep core to the outer corona, and the solar wind.
      
Three helioseismology instruments are providing unique data for the study of the structure and dynamics of the solar interior, from the very deep core to the outermost layers of the convection zone.
      
Twenty centimetres deep core samples were collected from undisturbed and recently disturbed intertidal mud.
      
Eggs were found throughout a 25 cm deep core but deeper than 20 cm they were very scarce.
      
Clay minerals in seven shallow water (100 to 600 m deep) dredged samples and in two deep-sea (3,000 to 5,000 m deep) core samples near West Antarctica were investigated by X-ray diffraction analyses.
      
Carbonates form a major proportion of the evaporites in a 23 m deep core and several dolomite-rich horizons are recorded.
      
The single sample of doubtful depth from Luna 20 shows a much lesser near-surface irradiation, giving results similar to those on the Apollo 12 core and the 54-80 depth sample from the Apollo 15 deep core.
      
 

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