Estimation of secular density variations in the upper atmosphere from 1964–2007 satellite drag data     

I. I. Volkov  A. I. Semenov  V. V. Suevalov 《Solar System Research》2011,45(5):420-432

Orbital parameters of several artificial satellites of the Earth were analyzed for 1964–2007 and secular variations of the atmospheric density were estimated for the last 30–40 years. The analysis was based on the information about orbital parameters of 17 satellites and high-precision numerical integrations of the equations of motion with allowance for basic perturbing factors and spatiotemporal density variations, calculated from measured solar activity indices using the NRLMSISE-00 atmosphere model. The results demonstrate the presence of long-term variations in the atmospheric density not presented in modern atmosphere models. During solar-activity cycle 21, the atmospheric density became 0.4 to 19% higher (depending on height) than in cycle 20. It decreased by 1.0 to 11% (depending on height) in cycle 22 as compared to cycle 21. Both decreases and increases were observed in the atmospheric density during cycle 23, but with much smaller gradients. The results cannot be explained only by the growing concentration of greenhouse gases. Possible causes of the density variations and possible ways to take them into account in modern empirical and semiempirical atmospheric models are discussed.  相似文献   

Dwarf copper-gold porphyry deposits of the Buchim-Damjan-Borov Dol ore district, Republic of Macedonia (FYROM)     

T. Serafimovski  V. Stefanova  A. V. Volkov 《Geology of Ore Deposits》2010,52(3):179-195

The metallogenic aspects, tectonic setting, magmatism, structure, and composition of Au- and Ag-bearing porphyry copper deposits in the Buchim-Damjan-Borov Dol ore district and their genetic features are considered and compared with earlier published data. Special attention is paid to supergene gold in heavy concentrate halos of the Borov Dol deposit. The total Cu reserves of the deposits discussed in this paper do not exceed 150 kt. The Buchim deposit likely is the world’s smallest deposit of this type currently involved in mining. A comprehensive study of these dwarf porphyry copper deposits is undertaken to answer questions on the conditions of their formation. How do they differ from formation conditions of giant deposits?  相似文献   

Eclipsing System PS UMa: Evolutionary Status and Physical Parameters of the Components     

I. M. Volkov  A. S. Kravtsova 《Astronomy Reports》2020,64(3):211-225

We present the first high accuracy UBVRI(RI)c CCD light curves of the newly discovered eclipsing system PS UMa = GSC 4375 1733 ($$P = 9_{·}^{d}27$$, $$V = 12_{·}^{m}42$$). The photometric solutions are found, the physical parameters of the components are derived. The eccentricity of the orbit was found to be negligible e = 0.074, which made it difficult to measure the rate of the apsidal rotation. High accuracy of our observations allowed us to find the reliable parameters of the system. Components (Sp = F7 + G1) have advanced significantly in their evolution, the age of the system is 2.4 billion years. The mass and the radius of G1 component is larger and it is ahead of the F7 component in its evolution. The model of the system best suits the theory in the absence of the overshooting in the core. Obtained from our observations photometrical parallax π = 0$$_{.}^{\prime\prime }$$00102(2) coincides with GAIA DR2 value $$\pi =0_{·}^{\prime\prime }00106(3)$$ within their errors. The new EW type variable with period $$ \approx {\kern 1pt} 0_{·}^{d}40$$ was found in the field of PS UMa.  相似文献