Zobrazeno 1 - 10
of 21
pro vyhledávání: '"O. A. Ozhogina"'
Autor:
A. A. Moykin, K. V. Shirshin, L. G. Lazareva, A. S. Medzhibovskiy, E. A. Bolshakova, O. R. Ozhogina, A. V. Shishulina
Publikováno v:
Plasticheskie massy. 1:45-47
The influence of the molecular weight and composition of polyalkyl (meth) acrylate thickeners on the properties NS-3 ultralow pour point naphthenic base oil (Nynas, Sweden) was determined. Using standard experimental techniques, it has been shown tha
Autor:
O. A. Ozhogina
Publikováno v:
Astronomy Letters. 45:627-634
On July 12, 2014, an unusual light structure was observed in the NOAA 12109 sunspot umbra at the Horizontal Solar Telescope of the Sayan Observatory. It differed from traditional light bridges in that it was entirely within the umbra without any appa
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:
Astronomy Letters. 41:848-858
The equivalent widths of six weak lines (7Li I, Si I, Fe I (two lines), Ti I, and CN) at the equatorial and polar limbs are compared. The lithium line is of greatest interest, because the abundance of lithium isotopes on the Sun and stars is closely
Autor:
O. A. Ozhogina
Publikováno v:
Астрономия-2018. Том 2.
Autor:
R. B. Teplitskaya, O. A. Ozhogina
Publikováno v:
Astronomy Letters. 40:361-371
The goal of this paper is a detailed statistical analysis of the low-frequency Ca II line intensity oscillations containing information about the dynamics of the lower and middle chromosphere. A pixel-by-pixel analysis of the observed parameters has
Autor:
O. A. Ozhogina, R. B. Teplitskaya
Publikováno v:
Astronomy Letters. 39:279-289
We have investigated 15 time series of Ca II line spectrograms in quiet-Sun regions located at various distances from the disk center. Our goal is to reveal the center-to-limb variation of the brightness oscillations. The residual intensities at the
Publikováno v:
Meditsina truda i promyshlennaia ekologiia. (4)
Functional reliability of engine operator and engine operator's assistant is one of the most important factors in railway safety. Ability to railway locomotive operation is determined via suitability criteria of occupationally important qualities of
Publikováno v:
Geomagnetism and Aeronomy. 50:831-842
The dynamic regime of eight regions in the quiet solar chromosphere was analyzed. Observations in CaII lines were performed with a moderate spatial resolution of around 2″. The purpose of this study was to compare the diagnostic capabilities of the
Publikováno v:
Solar Physics. 262:53-59
Observations of the central intensity of the Ca ii K and 849.8 nm lines are used to derive the ratios of the oscillation power in the frequency ranges of the “five-minute” (W5) and “three-minute” (W3) oscillations. It is shown that at high si