Zobrazeno 1 - 10
of 16
pro vyhledávání: '"S. A. Grigoryeva"'
Autor:
S. A. Grigoryeva, A. N. Kosyreva, T. F. Stepanova, K. B. Stepanova, I. V. Bakshtanovskaya, G. A. Kalgina, L. V. Kurlaeva
Publikováno v:
Инфекция и иммунитет, Vol 11, Iss 1, Pp 177-183 (2021)
The aim of the study was to identify a relationship between gene polymorphisms associated with developing coronary heart disease and pathogenetic features of opisthorchiasis invasion. There were compared laboratory parameters assessing the immune sys
Externí odkaz:
https://doaj.org/article/bd237ad60c7d4ade8b04f1199fa08ac2
Publikováno v:
Архивъ внутренней медицины, Vol 10, Iss 5, Pp 372-381 (2020)
Aim of the study. Evaluation of treatment adherence in patients with rheumatoid arthritis (RA) and comorbidity.Materials and methods. One hundred thirty-two women (mean age: 55.5 ± 10.5 years) with proven RA (mean duration of disease: 10.2 [4; 14] y
Externí odkaz:
https://doaj.org/article/4dc27d7f24844a06895edf6e461b9d44
Publikováno v:
Solar Physics. 291:1977-2002
We study Ca ii K profiles in structural features of the quiet chromosphere and plages using observations of two time series for two regions at the base of a coronal hole. One of the regions that we study has a low-brightness area where the reversal-f
Publikováno v:
Geomagnetism and Aeronomy. 49:884-890
It is difficult to numerically solve steady-state equations for calcium, which are used to determine temperature and electron density in a sunspot umbra chromosphere. As a result, the coefficients of equations, obtained using inversion of the measure
Autor:
S. A. Grigoryeva, R. B. Teplitskaya
Publikováno v:
Geomagnetism and Aeronomy. 49:916-926
The line profile inversion is as a rule used to model the atmosphere. The algorithm for determining the temperature and electron density in the middle chromosphere has been developed based on inversion of the profiles of five Ca II chromospheric line
Publikováno v:
Astronomy Reports. 53:569-577
The detailed measurements of Call K line profiles along a diameter of the solar disk are presented. The obtained limb-darkening curves are used to test three semi-empirical models for the quiet Sun assuming moderate resolution. The calculations were
Publikováno v:
Solar Physics. 195:269-279
Chemical composition anomalies of the corona and solar wind (FIP effect) have their origins in the chromosphere. We study the influence of the possible stratification of abundances in the chromosphere on the shape of corresponding strong Fraunhofer l
Autor:
S. A. Grigoryeva, I. P. Turova
Publikováno v:
Solar Physics. 197:43-56
The ratios I(K1)/I(H1) and I(K3)/I(H3) were calculated from four semi-empirical models of sunspot umbra. We determined the dependencies of both ratios of such parameters as temperature gradient and atmospheric opacity. A certain influence on the expe
Autor:
I. P. Turova, S. A. Grigoryeva
Publikováno v:
Solar Physics. 179:17-30
A comparison of theoretical and observed Caii H and K line profiles in sunspot umbrae has been made for different sunspot positions on the solar disk. Four semi-empirical static umbral models were used in calculations: the SUNSPOT model of Avrett (19
Publikováno v:
Krasnoyarsk Science. :223
Зазеркалье представляет собой особый тип бытия, связанный со сменой полярности, в результате чего модус жизни социального/личного прио