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Biomedical subjects

N Mandzhavidze

Publications and source records attributed to N Mandzhavidze.

2 recordsLinked to original sources

[Immunological parameters and ultrastructure of blood formed elements in nephrotic syndrome in children].

The aim of the study was the evaluation of significance of immunopathogenic mechanisms in the pathogenesis of minimal change nephrotic syndrome and the study of the ultrastructural changes of peripheral blood formed elements. The observation was carried out on 64 patients with steroid sensitive minimal change nephrotic syndrome. During the manifestation and recurrence of the disease, in the majority of the patients, the results of immunological studies revealed the reduction in both total and absolute count of T-lymphocytes on the background of decreased immunoregulatory index (T(4+)/ T(8+)). In the peripheral blood statistically reliable reduction in the percent value of T(3+) and T(4+) phenotype lymphocytes and elevation of number of T(8+)-lymphocytes were observed. On the background of normal values of B-lymphocytes appeared increase of IgM and decrease of IgG and IgA. In most cases significant elevation in the value of IgE - (244+10,3) and low values of INF-gamma, ultrastructural changes of blood monocytes were apparent. The peculiarities of ultrastructural changes of eosinophils and basophiles especially were pronounced by cytomembrane degranulation in form of decrease in electric density.

B-Lymphocytes↗

6Li from Solar Flares.

By introducing a hitherto ignored 6Li producing process, due to accelerated 3He reactions with 4He, we show that accelerated particle interactions in solar flares produce much more 6Li than 7Li. By normalizing our calculations to gamma-ray data, we demonstrate that the 6Li produced in solar flares, combined with photospheric 7Li, can account for the recently determined solar wind lithium isotopic ratio, obtained from measurements in lunar soil, provided that the bulk of the flare-produced lithium is evacuated by the solar wind. Further research in this area could provide unique information on a variety of problems, including solar atmospheric transport and mixing, solar convection and the lithium depletion issue, and solar wind and solar particle acceleration.

Journal Article↗