First Results of the Work of the All-Union Research Institute of Agricultural Economics

1958 ◽  
Vol 1 (4) ◽  
pp. 96-98
Author(s):  
V. Zhmuida
2013 ◽  
Vol 22 (4) ◽  
Author(s):  
M. Nechaeva ◽  
A. Antipenko ◽  
D. Bezrukov ◽  
Vl. Bezrukovs ◽  
A. Dementjev ◽  
...  

AbstractAn international VLBI experiment on radio location of the asteroid 2012 DA14 was organized on 2013 February 15–16, during its flyby close to Earth. The purpose of observations was to investigate and specify orbital parameters of the asteroid, as well as to evaluate its rotation period and other characteristics. The irradiation of the asteroid was performed by the RT-70 transmitter at Evpatoria (Crimea, Ukraine), while the reflected signals were successfully accepted by the two 32 m radio telescopes at Medicina (Bologna, Italy) and Irbene (Ventspils, Latvia). Processing and interpretation of the data were performed both in the Radiophysical Research Institute at Nizhny Novgorod and in the Ventspils International Radio Astronomy Center. The first results of this experiment are presented and discussed.


Author(s):  
Virag Szabó

The economic efficiency of cage and deep-litter farms of different sizes with a cost and income analysis based was examined on the 2004-2014 Farm Accountancy Data Network (FADN) data provided by the Hungarian Research Institute of Agricultural Economics (AKI). It was found that the differences in efficiency experienced in previous years continued to increase years after the cage changes in both types of hen keeping appeared. It has been shown that deep-litter farmers typically keep smaller stocks and 36% of stocks are supplied in the framework of family work, whose wages are not recorded as personal expenses. It was also found that both unit cost and average sales price per egg decrease in the case of the cage and the deep-litter method with the increase in farm size. While the second biggest decline in average sales price occurs in the case of cage farmers with a stock of over 25,000, in the case of deep-litter farmers it already comes about at a stock of over 10,000.


2012 ◽  
Vol 48 (No. 9) ◽  
pp. 425-432
Author(s):  
J. Kraus ◽  
Z. Sokol

This Article does not have an abstract.


2002 ◽  
Vol 153 (8) ◽  
pp. 293-297
Author(s):  
Jacqueline Gehrig-Fasel ◽  
Anton Bürgi

In order to assess the usefulness of a computer based silvicultural information system, the Swiss Federal Research Institute WSL, developed and tested a prototype of such a system in collaboration with the forest enterprise Bremgarten (BWW). This work describes the prototype, built on a GIS-platform, and fed with a database which particularly takes small mixed stands into account. First results are interpreted with regard to the usefulness of such a system in practice.


1976 ◽  
Vol 32 ◽  
pp. 577-588
Author(s):  
C. Mégessier ◽  
V. Khokhlova ◽  
T. Ryabchikova

My talk will be on the oblique rotator model which was first proposed by Stibbs (1950), and since received success and further developments. I shall present two different attempts at describing a star according to this model and the first results obtained in the framework of a Russian-French collaboration in order to test the precision of the two methods. The aim is to give the best possible representation of the element distributions on the Ap stellar surfaces. The first method is the mathematical formulation proposed by Deutsch (1958-1970) and applied by Deutsch (1958) to HD 125248, by Pyper (1969) to α2CVn and by Mégessier (1975) to 108 Aqr. The other one was proposed by Khokhlova (1974) and used by her group.


1976 ◽  
Vol 32 ◽  
pp. 109-116 ◽  
Author(s):  
S. Vauclair

This paper gives the first results of a work in progress, in collaboration with G. Michaud and G. Vauclair. It is a first attempt to compute the effects of meridional circulation and turbulence on diffusion processes in stellar envelopes. Computations have been made for a 2 Mʘstar, which lies in the Am - δ Scuti region of the HR diagram.Let us recall that in Am stars diffusion cannot occur between the two outer convection zones, contrary to what was assumed by Watson (1970, 1971) and Smith (1971), since they are linked by overshooting (Latour, 1972; Toomre et al., 1975). But diffusion may occur at the bottom of the second convection zone. According to Vauclair et al. (1974), the second convection zone, due to He II ionization, disappears after a time equal to the helium diffusion time, and then diffusion may happen at the bottom of the first convection zone, so that the arguments by Watson and Smith are preserved.


Author(s):  
H. Seiler ◽  
U. Haas ◽  
K.H. Körtje

The physical properties of small metal particles reveal an intermediate position between atomic and bulk material. Especially Ag has shown pronounced size effects. We compared silver layers evaporated in high vacuum with cluster layers of small silver particles, evaporated in N2 at a pressure of about 102 Pa. The investigations were performed by electron optical methods (TEM, SEM, EELS) and by Photoacoustic (PA) Spectroscopy (gas-microphone detection).The observation of cluster layers with TEM and high resolution SEM show small silver particles with diameters of about 50 nm (Fig. 1 and Figure 2, respectively). The electron diffraction patterns of homogeneous Ag layers and of cluster layers are similar, whereas the low loss EELS spectra due to plasmon excitation are quite different. Fig. 3 and Figure 4 show first results of EELS spectra of a cluster layer of small silver particles on carbon foil and of a homogeneous Ag layer, respectively.


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