MODEL OF FORMING OF PROFESSIONAL INTEGRATIVE- SERVICE COMPETENSE OF SPECIALIST OF INDUSTRY OF FEED AND HOSPITALITY

В статье показано, что индустрия питания и гостеприимства, развивается быстрыми темпами и нуждается в инновациях, способных поднять уровень услуг в соответствии с возрастающими требованиями потребителей. Соответственно появляется необходимость подготовки специалистов, имеющих фундаментальные, профессиональные знания в области индустрии питания и гостеприимства, стремящихся к творческой самореализации, так как эффективное внедрение любых инноваций невозможно при низкой квалификации персонала и его слабой мотивации. Рассмотренная авторами модель формирования профессиональной интегративно-сервисной компетенции будущего специалиста индустрии питания и гостеприимства в среднем профессиональном образовании, включает взаимосвязанные целевую, методическую и результативную составляющие, а также механизм контроля формирования данной компетенции.The article shows that the catering and hospitality industry, is growing rapidly and needs in innovation, capable of raising the level of services in accordance with the growing demands of consumers. Accordingly, there is need to train specialists with fundamental and professional knowledge in the field of catering and hospitality industry, striving for creative self-realization, as the effective implementation of any innovation is impossible for unskilled personnel and their weak motivation.Considered the authors model of integrative professional competence of the future expert service food and hospitality industry in the secondary vocational education, including related task, methodological and productive components, as well as a mechanism to monitor the formation of this competence

Results of observations of asteroids at the Russian–Turkish RTT-150 telescope from 2004–2013

© 2015, Allerton Press, Inc. We report the results of analysis of the data volume containing 13834 topocentric positions of 231 asteroids obtained from observations at the Russian–Turkish RTT-150 telescope (TÜBITAK (Scientific and Technological Research Council of Turkey), Turkey) in 2004–2013. The positions of asteroids were calculated with the differential reduction method in the ICRS system with the use of the reference catalogs of the UCAC series. The observational program covered the main-belt asteroids closely encountering the other asteroids and the near-Earth asteroids (NEA). For the main belt asteroids, the mean-square error of one position was 84 and 68 mas in right ascension and declination, respectively, while it was 160 and 120 mas, respectively, for NEAs. The obtained volume of the asteroid positions widens the arc of groundbased observations of these bodies, which is important for evaluating their orbital elements with a higher accuracy. Moreover, observations of the main-belt asteroids in the periods of close encounters yield valuable material to solve the problem on accurate estimation of the masses of asteroids with a dynamic method. It has been shown that the supplementing of the input dataset with the here-reported observational volume decreases the error in the estimates of the perturbing asteroid mass and the orbital parameters of perturbed bodies

Interleukin-1 activity in aged animals. Abstr.

© 2015, Allerton Press, Inc. We report the results of analysis of the data volume containing 13834 topocentric positions of 231 asteroids obtained from observations at the Russian–Turkish RTT-150 telescope (TÜBITAK (Scientific and Technological Research Council of Turkey), Turkey) in 2004–2013. The positions of asteroids were calculated with the differential reduction method in the ICRS system with the use of the reference catalogs of the UCAC series. The observational program covered the main-belt asteroids closely encountering the other asteroids and the near-Earth asteroids (NEA). For the main belt asteroids, the mean-square error of one position was 84 and 68 mas in right ascension and declination, respectively, while it was 160 and 120 mas, respectively, for NEAs. The obtained volume of the asteroid positions widens the arc of groundbased observations of these bodies, which is important for evaluating their orbital elements with a higher accuracy. Moreover, observations of the main-belt asteroids in the periods of close encounters yield valuable material to solve the problem on accurate estimation of the masses of asteroids with a dynamic method. It has been shown that the supplementing of the input dataset with the here-reported observational volume decreases the error in the estimates of the perturbing asteroid mass and the orbital parameters of perturbed bodies

Results of observations of asteroids at the Russian–Turkish RTT-150 telescope from 2004–2013

© 2015, Allerton Press, Inc. We report the results of analysis of the data volume containing 13834 topocentric positions of 231 asteroids obtained from observations at the Russian–Turkish RTT-150 telescope (TÜBITAK (Scientific and Technological Research Council of Turkey), Turkey) in 2004–2013. The positions of asteroids were calculated with the differential reduction method in the ICRS system with the use of the reference catalogs of the UCAC series. The observational program covered the main-belt asteroids closely encountering the other asteroids and the near-Earth asteroids (NEA). For the main belt asteroids, the mean-square error of one position was 84 and 68 mas in right ascension and declination, respectively, while it was 160 and 120 mas, respectively, for NEAs. The obtained volume of the asteroid positions widens the arc of groundbased observations of these bodies, which is important for evaluating their orbital elements with a higher accuracy. Moreover, observations of the main-belt asteroids in the periods of close encounters yield valuable material to solve the problem on accurate estimation of the masses of asteroids with a dynamic method. It has been shown that the supplementing of the input dataset with the here-reported observational volume decreases the error in the estimates of the perturbing asteroid mass and the orbital parameters of perturbed bodies