1,885 research outputs found

    Non-LTE treatment of molecules in the photospheres of cool stars

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    We present a technique to treat systems with very many levels, like molecules, in non-LTE. This method is based on a superlevel formalism coupled with rate operator splitting. Superlevels consist of many individual levels that are assumed to be in LTE relative to each other. The usage of superlevels reduces the dimensionality of the rate equations dramatically and, thereby, makes the problem computationally more easily treatable. Our superlevel formalism retains maximum accuracy by using direct opacity sampling (dOS) when calculating the radiative transitions and the opacities. We developed this method in order to treat molecules in cool dwarf model calculations in non-LTE. Cool dwarfs have low electron densities and a radiation field that is far from a black body radiation field, both properties may invalidate the conditions for the common LTE approximation. Therefore, the most important opacity sources, the molecules, need to be treated in non-LTE. As a case study we applied our method to carbon monoxide. We find that our method gives accurate results since the conditions for the superlevel method are very well met for molecules. Due to very high collisional cross sections with hydrogen, and the high densities of H_2 the population of CO itself shows no significant deviation from LTE.Comment: AASTeX v50, 35 pages including 12 figures, accepted by Ap

    Проект установки получения синтез-газа

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    ВКР 91 страницу, 6 рисунков, 40 таблиц, 24 литературных источника. Ключевые слова: синтез-газ, конверсия, применение синтез-газа, сырье, природный газ, технологическая схема, производство, метан, метанол. Объект разработки: производство синтез-газа методом паровой каталитической конверсии природного газа. Цель работы: изучение всех физико - химических свойств процесса и их влияния на протекание реакции, а также конструирование основного аппарата установки получения синтез - газа. В результате исследования выполнен расчет материального и теплового балансов, также конструктивный и механический расчеты, на основании которых был выполнен чертеж основного аппарата. ВКР выполнена на кафедре ТОВПМ ст. группы 2Д2А Якимовой В.А., под руководством к.х.н. Мананковой А.А.The final qualifying work contains 91 page, 6 figures, 40 tables and 24 literature sources. Content words are conversion, synthesis gas. The object of the development is the production of synthesis gas by catalytic steam reforming of natural gas. The mission is the study of physical - chemical properties of the process and their influence on the reaction, as well as the construction of the main unit installation producing synthesis - gas. The study was carried out payment of material and heat balances, the constructive and mechanical calculations, drawing on the basis of which the main unit was made. The final qualifying work carried out at the Department of TOVPM student group 2D2A Vera Yakimova, under the leadership of Candidate of Chemical Sciences Ann Manankova

    Spectral Properties of Brown Dwarfs and Hot Jupiters

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    Brown dwarfs bridge the gap between the stellar and planetary mass regimes. Evolving from conditions very similar to the lowest-mass stars, the atmospheres of older brown dwarfs closely resemble those expected in close-in extrasolar giant planets, and with cooler BDs still being discovered, more and more approach the properties of gas giants at wider separation. Interpreting the spectra of BDs is therefore a crucial step towards understanding and predicting the spectral and thermal properties of EGPs. Essential properties of substellar atmospheres are massive molecular line-blanketing and the condensation of species with decreasing Teff, changing the chemical equilibrium composition and causing absorption from dust grains. More complex details involve the distribution of dust clouds over the surface giving rise to temporal variability, and possible deviations from chemical equilibrium conditions. In the case of close-in EGPs and some BDs in binary systems, the effect of irradiation from the primary significantly affects the spectral properties and thermal evolution.Comment: 12 pages, 6 figures, Review to be published in "High Resolution Infrared Spectroscopy in Astronomy", Proceedings of the ESO Workshop Held in Garching, Germany, 18-21 Nov., 2003, eds. H.U. Kaeufl, R. Siebenmorgen, & A. Moorwood, ESO Astrophysics Symposia http://www.eso.org/gen-fac/meetings/ekstasy2003

    Обоснование выбора электродвигателя и схемы его включения для системы точного поддержания скорости

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    Рассматривается применение в системах точного поддержания скорости различных синхронных электродвигателей. В результате сравнения рекомендовано применение в таких системах конденсаторного синхронного реактивного двигателя с трехфазными обмотками статора. Это позволяет упростить и удешевить систему точного электропривода и повысить ее надежность

    Non-LTE Effects of Na I in the Atmosphere of HD209458b

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    The recent announcement that sodium absorption has been observed in the atmosphere of HD209458b, the only EGP observed to transit its parent star, is the first direct detection of an EGP atmosphere. We explore the possibility that neutral sodium is {\em not} in local thermodynamic equilibrium (LTE) in the outer atmosphere of irradiated EGPs and that the sodium concentration may be underestimated by models that make the LTE assumption. Our results indicate that it may not be necessary to invoke excessive photoionization, low metallicity, or even high altitude clouds to explain the observations
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