A Study of X-Ray Negative Dyspepsia with Reference to Histologic Changes in the Gastric Mucosa

1957 ◽  
Vol 32 (2) ◽  
pp. 313-324 ◽  
Author(s):  
M. Shiner ◽  
I. Doniach
Science ◽  
1950 ◽  
Vol 111 (2885) ◽  
pp. 379-380 ◽  
Author(s):  
A. Engstrom ◽  
D. Glick

2002 ◽  
Vol 70 (5) ◽  
pp. 2630-2639 ◽  
Author(s):  
Y. Zavros ◽  
G. Rieder ◽  
Amy Ferguson ◽  
J. L. Merchant

ABSTRACT In mouse models and humans, Helicobacter pylori is associated with an increase in serum gastrin and gastrin-expressing (G) cells with a concomitant decrease in somatostatin-expressing D cells. Inflammation of the gastric mucosa can progress to metaplastic changes in the stomach and to decreased colonization by H. pylori and increased colonization by non-H. pylori organisms. In addition, about 20% of individuals with chronic gastritis are H. pylori negative, suggesting that other organisms may induce gastritis. Consistent with this hypothesis, we report here that Acinetobacter lwoffii causes the same histologic changes as does H. pylori. Gastric epithelial cells were isolated from the entire stomach by an enzymatic method for quantitation by both flow cytometry and morphometric analysis. Two months after mice were inoculated with H. pylori or A. lwoffii, the mucosal T- and B-cell numbers significantly increased. After 4 months of infection, there was a threefold increase in the number of G cells and a doubling in the number of parietal cells. A threefold decrease in the number of D cells occurred in H. pylori- and A. lwoffii-infected mice. Plasma gastrin levels increased after both H. pylori and A. lwoffii infection. Histology revealed the presence of inflammation in the gastric mucosa with both A. lwoffii and H. pylori infection. A periodic acid-Schiff stain-alcian blue stain revealed mucous gland metaplasia of the corpus. Collectively, the results demonstrate that gastritis and hypergastrinemia are not specific for H. pylori but can be induced by other gram-negative bacteria capable of infecting the mouse stomach.


1937 ◽  
Vol 33 (10) ◽  
pp. 1178-1184
Author(s):  
E. A. Kamensky

The study of the relief of the mucous membrane of the stomach and intestines made it possible to expand and clarify the X-ray diagnosis with earlier and more subtle X-ray data. However, these data are still not widely used in order to capture the evolution of a particular physiological or pathological process (Reinberg, Stern, Rothermel). Still underestimated is the tremendous help they can provide in accounting for the effectiveness of treatment.


1999 ◽  
Vol 2 (4) ◽  
pp. 215-220 ◽  
Author(s):  
Carlos A. Rubio ◽  
Yo Kato ◽  
Akio Yanagisawa ◽  
Yasuo Ninomiya ◽  
Koichi Mandai

1994 ◽  
Vol 144 ◽  
pp. 275-277
Author(s):  
M. Karlický ◽  
J. C. Hénoux

AbstractUsing a new ID hybrid model of the electron bombardment in flare loops, we study not only the evolution of densities, plasma velocities and temperatures in the loop, but also the temporal and spatial evolution of hard X-ray emission. In the present paper a continuous bombardment by electrons isotropically accelerated at the top of flare loop with a power-law injection distribution function is considered. The computations include the effects of the return-current that reduces significantly the depth of the chromospheric layer which is evaporated. The present modelling is made with superthermal electron parameters corresponding to the classical resistivity regime for an input energy flux of superthermal electrons of 109erg cm−2s−1. It was found that due to the electron bombardment the two chromospheric evaporation waves are generated at both feet of the loop and they propagate up to the top, where they collide and cause temporary density and hard X-ray enhancements.


1994 ◽  
Vol 144 ◽  
pp. 1-9
Author(s):  
A. H. Gabriel

The development of the physics of the solar atmosphere during the last 50 years has been greatly influenced by the increasing capability of observations made from space. Access to images and spectra of the hotter plasma in the UV, XUV and X-ray regions provided a major advance over the few coronal forbidden lines seen in the visible and enabled the cooler chromospheric and photospheric plasma to be seen in its proper perspective, as part of a total system. In this way space observations have stimulated new and important advances, not only in space but also in ground-based observations and theoretical modelling, so that today we find a well-balanced harmony between the three techniques.


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